徳島大学 / 教育研究者総覧 --- 古屋玲 S.

個人のホームページ

https://researchmap.jp/rsf (researchmap)

専門分野

○	天文学 (Astronomy)

研究テーマ

○	(電波天文学, 赤外線天文学, 星形成過程, 星間物質, 銀河の進化, 分子や原子輝線の励起機構, 偏波観測, データ処理アルゴリズム, 星間ダスト, 次世代直線偏波撮像装置SCUBA-3の開発, 大型サブミリ波望遠鏡LSTの建設)

著書・論文

著書:

1.	石丸善康, 伊藤伸一, 宇野剛史, 岡村康弘, 大平健司, 小野公輔, 掛井秀一, 金西計英, 澤田麻衣子, 蓮沼徹, 古屋 S. 玲, 松浦健二, 松本和幸, 土岐順子, 阿部香織, 山﨑紅, 辰巳丈夫, 勝村幸博 : 情報科学入門, 日経BP社, 東京, 2019年4月.
2.	石丸善康, 伊藤伸一, 宇野剛史, 岡村康弘, 大平健司, 小野公輔, 掛井秀一, 金西計英, 澤田麻衣子, 蓮沼徹, 古屋 S. 玲, 松浦健二, 松本和幸, 土岐順子, 阿部香織, 山﨑紅, 辰巳丈夫, 勝村幸博 : 情報科学入門, 日経BP社, 東京, 2018年4月.
3.	石丸善康, 伊藤伸一, 宇野剛史, 岡村康弘, 大平健司, 小野公輔, 掛井秀一, 金西計英, 澤田麻衣子, 蓮沼徹, 古屋 S. 玲, 松浦健二, 松本和幸, 土岐順子, 阿部香織, 山﨑紅, 辰巳丈夫, 勝村幸博 : 情報科学入門, 日経BP社, 東京, 2017年4月.
4.	デレクワード=トンプソン, アンソニー P ウィットワース, 古屋 S. 玲 : ワード-トンプソン&ウィットワース星形成論―銀河進化における役割から惑星系の誕生まで, --- 翻訳 ---, 丸善出版, ISBN-13: 978-4621087367, 全404ページ, https://www.maruzen-publishing.co.jp/item/b294462.html,, 東京, 2016年6月. (要約) 星(恒星)には一生があり，誕生したての若い星から晩年の年老いた星まで，われわれが眺める星空にはさまざまな様相で瞬いている．星は，星間物質と呼ばれる宇宙を漂うガス雲と固体の細かい塵である星間塵(宇宙塵)によって形成され，ガス雲のとくに高密度部分(分子雲)が回転しながら集まり収縮することで円盤状となり，その中心に星の赤ちゃんというべき原始星が誕生する．その後，星は成長し瞬き，晩年を迎えると膨張して超新星爆発や白色矮星となって生涯を終える．本書はそんな星の一生の中でも，誕生(形成)過程における理論や観測研究に関して，90年代から2000年代までの進展をまとめている．原著者は星形成に関する第一人者で，日本では星形成に関してしっかりとまとめた書籍はなく，これから星形成を学びたいと考えている学生に最適の一冊．

学術論文(審査論文):

1.	Derek Ward-Thompson, Janik Karoly, Kate Pattle, Anthony Whitworth, Jason Kirk, David Berry, Pierre Bastien, Tao-Chung Ching, Simon Coudé, Jihye Hwang, Woojin Kwon, Archana Soam, Jia-Wei Wang, Tetsuo Hasegawa, Shih-Ping Lai, Keping Qiu, Doris Arzoumanian, Tyler L. Bourke, Do-Young Byun, Huei-Ru Vivien Chen, Wen Ping Chen, Mike Chen, Zhiwei Chen, Jungyeon Cho, Minho Choi, Youngwoo Choi, Yunhee Choi, Antonio Chrysostomou, Eun Jung Chung, Sophia Dai, Victor Debattista, James Di Francesco, Pham Ngoc Diep, Yasuo Doi, Hao-Yuan Duan, Yan Duan, Chakali Eswaraiah, Lapo Fanciullo, Jason Fiege, Laura M. Fissel, Erica Franzmann, Per Friberg, Rachel Friesen, Gary Fuller, Ray S. Furuya, Tim Gledhill, Sarah Graves, Jane Greaves, Matt Griffin, Qilao Gu and at. al : First BISTRO Observations of the Dark Cloud Taurus L1495A-B10: The Role of the Magnetic Field in the Earliest Stages of Low-mass Star Formation, The Astrophysical Journal, Vol.946, No.2, id.62, 2023. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/acbea4 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85151821532 (DOI: 10.3847/1538-4357/acbea4, Elsevier: Scopus)
2.	Sakiko Fukaya, Hiroko Shinnaga, Ray S. Furuya, Kohji Tomisaka, Masahiro N Machida and Naoto Harada : Twisted magnetic field in star formation processes of L1521 F revealed by submillimeter dual-band polarimetry using the James Clerk Maxwell Telescope, Publications of the Astronomical Society of Japan, Vol.75, No.1, 120-127, 2023. (出版サイトへのリンク) ● Publication site (DOI): 10.1093/pasj/psac094 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85150472652 (DOI: 10.1093/pasj/psac094, Elsevier: Scopus)
3.	Mehrnoosh Tahani, Pierre Bastien, Ray S. Furuya, Kate Pattle, Doug Johnstone, Doris Arzoumanian, Yasuo Doi, Tetsuo Hasegawa, Shu-ichiro Inutsuka, Simon Coudé, Laura Fissel, Michael Chun-Yuan Chen, Frédérick Poidevin, Sarah Sadavoy, Rachel Friesen, Patrick M. Koch, James Di Francesco, Gerald H. Moriarty-Schieven, Zhiwei Chen, Eun Jung Chung, Chakali Eswaraiah, Lapo Fanciullo, Tim Gledhill, Valentin Le M. J. Gouellec, Thiem Hoang, Jihye Hwang, Ji-hyun Kang, Kyoung Hee Kim, Florian Kirchschlager, Woojin Kwon, Chang Won Lee, Hong-Li Liu, Takashi Onaka, Mark G. Rawlings, Archana Soam, Motohide Tamura, Xindi Tang, Kohji Tomisaka, Anthony P. Whitworth, Jungmi Kwon, Thuong D. Hoang, Matt Redman, David Berry, Tao-Chung Ching, Jia-Wei Wang, Shih-Ping Lai, Keping Qiu, Derek Ward-Thompson, Martin Houde, Do-Young Byun and at. al : JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with NGC 6334, The Astrophysical Journal, Vol.944, No.2, id.139, 2023. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/acac81 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85148856351 (DOI: 10.3847/1538-4357/acac81, Elsevier: Scopus)
4.	Tao-Chung Ching, Keping Qiu, Di Li, Zhiyuan Ren, Shih-Ping Lai, David Berry, Kate Pattle, Ray S. Furuya, Derek Ward-Thompson, Doug Johnstone, Patrick M. Koch, Chang Won Lee, Thiem Hoang, Tetsuo Hasegawa, Woojin Kwon, Pierre Bastien, Chakali Eswaraiah, Jia-Wei Wang, Kyoung Hee Kim, Jihye Hwang, Archana Soam, A-Ran Lyo, Junhao Liu, Valentin Le M. J. Gouellec, Doris Arzoumanian, Anthony Whitworth, James Di Francesco, Frédérick Poidevin, Tie Liu, Simon Coudé, Mehrnoosh Tahani, Hong-Li Liu, Takashi Onaka, Dalei Li, Motohide Tamura, Zhiwei Chen, Xindi Tang, Florian Kirchschlager, Tyler L. Bourke, Do-Young Byun, Mike Chen, Huei-Ru Vivien Chen, Wen Ping Chen, Jungyeon Cho, Yunhee Choi, Youngwoo Choi, Minho Choi, Antonio Chrysostomou, Eun Jung Chung, Y. Sophia Dai and at al : The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 Filament, The Astrophysical Journal, Vol.941, No.2, id122, 2022. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/ac9dfb (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85145393150 (DOI: 10.3847/1538-4357/ac9dfb, Elsevier: Scopus)
5.	Jihye Hwang, Jongsoo Kim, Kate Pattle, Chang Won Lee, Patrick M. Koch, Doug Johnstone, Kohji Tomisaka, Anthony Whitworth, Ray S. Furuya, Ji-hyun Kang, A-Ran Lyo, Eun Jung Chung, Doris Arzoumanian, Geumsook Park, Woojin Kwon, Shinyoung Kim, Motohide Tamura, Jungmi Kwon, Archana Soam, Ilseung Han, Thiem Hoang, Kyoung Hee Kim, Takashi Onaka, Eswaraiah Chakali, Derek Ward-Thompson, Liu Hong-Li, Xindi Tang, Wen Ping Chen, Masafumi Matsumura, Thuong Duc Hoang, Zhiwei Chen, Valentin Le M. J. Gouellec, Florian Kirchschlager, Fr erick ed Poidevin, Pierre Bastien, Keping Qiu, Tetsuo Hasegawa, Shih-Ping Lai, Do-Young Byun, Jungyeon Cho, Minho Choi, Youngwoo Choi, Yunhee Choi, Il-Gyo Jeong, Miju Kang, Hyosung Kim, Kee-tae Kim, Jeong-Eun Lee, Sang-sung Lee, Yong-Hee Lee and et al. : The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2, The Astrophysical Journal, Vol.941, No.1, id.51, 2022. (要約) We present and analyze observations of polarized dust emission at 850 μm toward the central 1 × 1 pc hub-filament structure of Monoceros R2 (Mon R2). The data are obtained with SCUBA-2/POL-2 on the James Clerk Maxwell Telescope (JCMT) as part of the B-fields in Star-forming Region Observations survey. The orientations of the magnetic field follow the spiral structure of Mon R2, which are well described by an axisymmetric magnetic field model. We estimate the turbulent component of the magnetic field using the angle difference between our observations and the best-fit model of the underlying large-scale mean magnetic field. This estimate is used to calculate the magnetic field strength using the Davis Chandrasekhar Fermi method, for which we also obtain the distribution of volume density and velocity dispersion using a column density map derived from Herschel data and the C¹⁸O (J = 3 - 2) data taken with HARP on the JCMT, respectively. We make maps of magnetic field strengths and mass-to-flux ratios, finding that magnetic field strengths vary from 0.02 to 3.64 mG with a mean value of 1.0 ± 0.06 mG, and the mean critical mass-to-flux ratio is 0.47 ± 0.02. Additionally, the mean Alfvén Mach number is 0.35 ± 0.01. This suggests that, in Mon R2, the magnetic fields provide resistance against large-scale gravitational collapse, and the magnetic pressure exceeds the turbulent pressure. We also investigate the properties of each filament in Mon R2. Most of the filaments are aligned along the magnetic field direction and are magnetically subcritical. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/ac99e0 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85144795071 (DOI: 10.3847/1538-4357/ac99e0, Elsevier: Scopus)
6.	Kate Pattle, Shih-Ping Lai, Sarah Sadavoy, Simon Coudé, Sebastian Wolf, Ray S. Furuya, Woojin Kwon, Chang Won Lee and Niko Zielinski : Magnetic fields and outflows in the large Bok globule CB 54, Monthly Notices of the Royal Astronomical Society, Vol.515, No.1, 1026, 2022. (徳島大学機関リポジトリ) ● Metadata: 117848 (出版サイトへのリンク) ● Publication site (DOI): 10.1093/mnras/stac1356 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1093/mnras/stac1356 (徳島大学機関リポジトリ: 117848, DOI: 10.1093/mnras/stac1356)
7.	Lapo Fanciullo, Francisca Kemper, Kate Pattle, Patrick M Koch, Sarah Sadavoy, Simon Coudé, Archana Soam, Thiem Hoang, Takashi Onaka, Valentin Le M J Gouellec, Doris Arzoumanian, David Berry, Chakali Eswaraiah, Eun Jung Chung, Ray S. Furuya, Charles H L Hull, Jihye Hwang, Douglas Johnstone, Ji-hyun Kang, Kyoung Hee Kim, Florian Kirchschlager, Könyves Vera, Jungmi Kwon, Woojin Kwon, Shih-Ping Lai, Chang Won Lee, Tie Liu, A-Ran Lyo, Ian Stephens, Motohide Tamura, Xindi Tang, Derek Ward-Thompson, Anthony Whitworth and Hiroko Shinnaga : The JCMT BISTRO Survey: multiwavelength polarimetry of bright regions in NGC 2071 in the far-infrared/submillimetre range, with POL-2 and HAWC+, Monthly Notices of the Royal Astronomical Society, Vol.512, No.2, 1985-2002, 2022. (要約) Polarized dust emission is a key tracer in the study of interstellar medium and of star formation. The observed polarization, however, is a product of magnetic field structure, dust grain properties, and grain alignment efficiency, as well as their variations in the line of sight, making it difficult to interpret polarization unambiguously. The comparison of polarimetry at multiple wavelengths is a possible way of mitigating this problem. We use data from HAWC+ /SOFIA and from SCUBA-2/POL-2 (from the BISTRO survey) to analyse the NGC 2071 molecular cloud at 154, 214, and 850 μ m. The polarization angle changes significantly with wavelength over part of NGC 2071, suggesting a change in magnetic field morphology on the line of sight as each wavelength best traces different dust populations. Other possible explanations are the existence of more than one polarization mechanism in the cloud or scattering from very large grains. The observed change of polarization fraction with wavelength, and the 214-to-154 μ m polarization ratio in particular, are difficult to reproduce with current dust models under the assumption of uniform alignment efficiency. We also show that the standard procedure of using monochromatic intensity as a proxy for column density may produce spurious results at HAWC+wavelengths. Using both long-wavelength (POL-2, 850 μ m) and short-wavelength (HAWC+, ≲200μ m) polarimetry is key in obtaining these results. This study clearly shows the importance of multi-wavelength polarimetry at submillimetre bands to understand the dust properties of molecular clouds and the relationship between magnetic field and star formation. (出版サイトへのリンク) ● Publication site (DOI): 10.1093/mnras/stac528 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85128507405 (DOI: 10.1093/mnras/stac528, Elsevier: Scopus)
8.	Woojin Kwon, Kate Pattle, Sarah Sadavoy, Charles H. L. Hull, Doug Johnstone, Derek Ward-Thompson, James Di Francesco, Patrick M. Koch, Ray S. Furuya, Yasuo Doi and et al. : B-fields in Star-forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens Main, The Astrophysical Journal, Vol.926, No.2, 163, 2022. (要約) We present 850 μm polarimetric observations toward the Serpens Main molecular cloud obtained using the POL-2 polarimeter on the James Clerk Maxwell Telescope as part of the B-fields In STar-forming Region Observations survey. These observations probe the magnetic field morphology of the Serpens Main molecular cloud on about 6000 au scales, which consists of cores and six filaments with different physical properties such as density and star formation activity. Using the histogram of relative orientation (HRO) technique, we find that magnetic fields are parallel to filaments in less-dense filamentary structures where ${N}_{{{m{H}}}_{2}}t 0.93imes {10}^{22}$ cm-2 (magnetic fields perpendicular to density gradients), while they are perpendicular to filaments (magnetic fields parallel to density gradients) in dense filamentary structures with star formation activity. Moreover, applying the HRO technique to denser core regions, we find that magnetic field orientations change to become perpendicular to density gradients again at ${N}_{{{m{H}}}_{2}}pprox 4.6imes {10}^{22}$ cm-2. This can be interpreted as a signature of core formation. At ${N}_{{{m{H}}}_{2}}pprox 16imes {10}^{22}$ cm-2, magnetic fields change back to being parallel to density gradients once again, which can be understood to be due to magnetic fields being dragged in by infalling material. In addition, we estimate the magnetic field strengths of the filaments (BPOS = 60 300 μG)) using the Davis Chandrasekhar Fermi method and discuss whether the filaments are gravitationally unstable based on magnetic field and turbulence energy densities. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/ac4bbe (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85125701679 (DOI: 10.3847/1538-4357/ac4bbe, Elsevier: Scopus)
9.	Yasuo Doi, Kohji Tomisaka, Tetsuo Hasegawa, Simon Coudé, Doris Arzoumanian, Pierre Bastien, Masafumi Matsumura, Mehrnoosh Tahani, Sarah Sadavoy, Charles H. L. Hull, Doug Johnstone, James Di Francesco, Yoshito Shimajiri, Ray S. Furuya, Jungmi Kwon, Motohide Tamura, Derek Ward-Thompson, Valentin Le M. J. Gouellec, Thiem Hoang, Florian Kirchschlager, Jihye Hwang, Chakali Eswaraiah, Patrick M. Koch, Anthony P. Whitworth, Kate Pattle, Woojin Kwon, Jihyun Kang, Shu-ichiro Inutsuka, Tyler L. Bourke, Xindi Tang, Lapo Fanciullo, Chang Won Lee, Hong-Li Liu, A-Ran Lyo, Keping Qiu and Shih-Ping Lai : The JCMT BISTRO Survey: Evidence for Pinched Magnetic Fields in Quiescent Filaments of NGC 1333, The Astrophysical Journal Letters, Vol.923, No.1, 923, 2021. (要約) We investigate the internal 3D magnetic structure of dense interstellar filaments within NGC 1333 using polarization data at 850 μm from the B-fields In STar-forming Region Observations survey at the James Clerk Maxwell Telescope. Theoretical models predict that the magnetic field lines in a filament will tend to be dragged radially inward (i.e., pinched) toward the central axis due to the filament's self-gravity. We study the cross-sectional profiles of the total intensity (I) and polarized intensity (PI) of dust emission in four segments of filaments unaffected by local star formation that are expected to retain a pristine magnetic field structure. We find that the filaments' FWHMs in PI are not the same as those in I, with two segments being appreciably narrower in PI (FWHM ratio ≃0.7 0.8) and one segment being wider (FWHM ratio ≃1.3). The filament profiles of the polarization fraction (P) do not show a minimum at the spine of the filament, which is not in line with an anticorrelation between P and I normally seen in molecular clouds and protostellar cores. Dust grain alignment variation with density cannot reproduce the observed P distribution. We demonstrate numerically that the I and PI cross-sectional profiles of filaments in magnetohydrostatic equilibrium will have differing relative widths depending on the viewing angle. The observed variations of FWHM ratios in NGC 1333 are therefore consistent with models of pinched magnetic field structures inside filaments, especially if they are magnetically near-critical or supercritical. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/2041-8213/ac3cc1 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85122460749 (DOI: 10.3847/2041-8213/ac3cc1, Elsevier: Scopus)
10.	A-Ran Lyo, Jongsoo Kim, Sarah Sadavoy, Doug Johnstone, David Berry, Kate Pattle, Woojin Kwon, Pierre Bastien, Takashi Onaka, James Di Francesco, Ji-Hyun Kang, Ray S. Furuya, Charles H. L. Hull, Motohide Tamura, Patrick M. Koch, Derek Ward-Thompson, Tetsuo Hasegawa, Thiem Hoang, Doris Arzoumanian, Chang Won Lee and et.al : The JCMT BISTRO Survey: An 850/450 μm Polarization Study of NGC 2071IR in Orion B, The Astrophysical Journal, Vol.918, No.2, 85, 2021. (要約) We present the results of simultaneous 450 μm and 850 μm polarization observations toward the massive star-forming region NGC 2071IR, a target of the BISTRO (B-fields in STar-forming Region Observations) Survey, using the POL-2 polarimeter and SCUBA-2 camera mounted on the James Clerk Maxwell Telescope. We find a pinched magnetic field morphology in the central dense core region, which could be due to a rotating toroidal disklike structure and a bipolar outflow originating from the central young stellar object IRS 3. Using the modified Davis-Chandrasekhar-Fermi method, we obtain a plane-of-sky magnetic field strength of 563 ± 421 μG in the central ~0.12 pc region from 850 μm polarization data. The corresponding magnetic energy density of 2.04 × 10-8 erg cm-3 is comparable to the turbulent and gravitational energy densities in the region. We find that the magnetic field direction is very well aligned with the whole of the IRS 3 bipolar outflow structure. We find that the median value of polarization fractions is 3.0% at 450 μm in the central 3' region, which is larger than the median value of 1.2% at 850 μm. The trend could be due to the better alignment of warmer dust in the strong radiation environment. We also find that polarization fractions decrease with intensity at both wavelengths, with slopes, determined by fitting a Rician noise model of 0.59 ± 0.03 at 450 μm and 0.36 ± 0.04 at 850 μm, respectively. We think that the shallow slope at 850 μm is due to grain alignment at the center being assisted by strong radiation from the central young stellar objects. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/ac0ce9 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85115928759 (DOI: 10.3847/1538-4357/ac0ce9, Elsevier: Scopus)
11.	Jihye Hwang, Jongsoo Kim, Kate Pattle, Woojin Kwon, Sarah Sadavoy, M. Patrick Koch, H. Charles L. Hull, Doug Johnstone, Ray S. Furuya, Chang Lee Won, Doris Arzoumanian, Mehrnoosh Tahani, Chakali Eswaraiah, Tie Liu, Florian Kirchschlager, Kee-Tae Kim, Motohide Tamura, Jungmi Kwon, -Ran A. Lyo, Archana Soam, Ji-hyun Kang, L. Tyler Bourke, Masafumi Matsumura, Steve Mairs, Gwanjeong Kim, Geumsook Park, Fumitaka Nakamura, Takashi Onaka, Xindi Tang, Hong-Li Liu, Derek Ward-Thompson, Di Li, Thiem Hoang, Tetsuo Hasegawa, Keping Qiu, Shih-Ping Lai and Pierre Bastien : The JCMT BISTRO Survey: The Distribution of Magnetic Field Strengths toward the OMC-1 Region, The Astrophysical Journal, Vol.913, No.2, 85, 2021. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/abf3c4 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85107792604 (DOI: 10.3847/1538-4357/abf3c4, Elsevier: Scopus)
12.	Yasuo Doi, Tetsuo Hasegawa, Pierre Bastien, Mehrnoosh Tahani, Doris Arzoumanian, Simon Coudé, Masafumi Matsumura, Sarah Sadavoy, H. Charles L. Hull, Yoshito Shimajiri, Ray S. Furuya, Doug Johnstone, Rene Plume, Shu-ichiro Inutsuka, Jungmi Kwon and Motohide Tamura : Two-component Magnetic Field along the Line of Sight to the Perseus Molecular Cloud: Contribution of the Foreground Taurus Molecular Cloud, The Astrophysical Journal, Vol.914, No.2, 122, 2021. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/abfcc5 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.3847/1538-4357/abfcc5 (DOI: 10.3847/1538-4357/abfcc5)
13.	Chakali Eswaraiah, Di Li, Ray S. Furuya, Tetsuo Hasegawa, Derek Ward-Thompson, Keping Qiu, Nagayoshi Ohashi, Kate Pattle, Sarah Sadavoy, H. Charles L. Hull, David Berry, Yasuo Doi, Tao-Chung Ching, Shih-Ping Lai, Jia-Wei Wang, M. Patrick Koch, Jungmi Kwon, Woojin Kwon, Pierre Bastien, Doris Arzoumanian, Simon Coudé, Archana Soam, Lapo Fanciullo, Hsi-Wei Yen, Junhao Liu, Thiem Hoang, Wen Chen Ping, Yoshito Shimajiri, Tie Liu, Zhiwei Chen, Hua-bai Li, -Ran A. Lyo, Jihye Hwang, Doug Johnstone, Ramprasad Rao, Nguyen Ngoc Bich, Pham Diep Ngoc, Steve Mairs, Harriet Parsons, Motohide Tamura, Mehrnoosh Tahani, Huei-Ru Chen Vivien, Fumitaka Nakamura, Hiroko Shinnaga, Ya-Wen Tang, Jungyeon Cho, Chang Lee Won, Shu-ichiro Inutsuka, Tsuyoshi Inoue, Kazunari Iwasaki and 95 more : The JCMT BISTRO Survey: Revealing the Diverse Magnetic Field Morphologies in Taurus Dense Cores with Sensitive Submillimeter Polarimetry, The Astrophysical Journal Letters, Vol.912, No.2, L27, 2021. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/2041-8213/abeb1c (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85106322742 (DOI: 10.3847/2041-8213/abeb1c, Elsevier: Scopus)
14.	Vera Könyves, Derek Ward-Thompson, Kate Pattle, James Francesco Di, Doris Arzoumanian, Zhiwei Chen, Ngoc Pham Diep, Chakali Eswaraiah, Lapo Fanciullo, Ray S. Furuya, Thiem Hoang, H. Charles L. Hull, Jihye Hwang, Doug Johnstone, Ji-hyun Kang, Janik Karoly, Florian Kirchschlager, M. Jason Kirk, M. Patrick Koch, Jungmi Kwon, Won Chang Lee, Takashi Onaka, Jean-François Robitaille, Archana Soam, Mehrnoosh Tahani, Xindi Tang, Motohide Tamura, David Berry, Pierre Bastien, Tao-Chung Ching, Simon Coudé, Woojin Kwon, Jia-Wei Wang, Tetsuo Hasegawa, Shih-Ping Lai and Keping Qiu : The JCMT BISTRO-2 Survey: The Magnetic Field in the Center of the Rosette Molecular Cloud, The Astrophysical Journal, Vol.913, No.1, 57, 2021. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/abf3ca (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85107316017 (DOI: 10.3847/1538-4357/abf3ca, Elsevier: Scopus)
15.	Kate Pattle, Shih-Ping Lai, Melvyn Wright, Simon Coudé, Richard Plambeck, Thiem Hoang, Ya-Wen Tang, Pierre Bastien, Chakali Eswaraiah, Ray S. Furuya, Jihye Hwang, Shu-ichiro Inutsuka, Kee-Tae Kim, Florian Kirchschlager, Woojin Kwon, Won Chang Lee, Sheng-Yuan Liu, Aran Lyo, Nagayoshi Ohashi, G. Mark Rawlings, Mehrnoosh Tahani, Motohide Tamura, Archana Soam, Jia-Wei Wang and Derek Ward-Thompson : OMC-1 dust polarization in ALMA Band 7: diagnosing grain alignment mechanisms in the vicinity of Orion Source I, Monthly Notices of the Royal Astronomical Society, Vol.503, No.3, 3414-3433, 2021. (徳島大学機関リポジトリ) ● Metadata: 116823 (出版サイトへのリンク) ● Publication site (DOI): 10.1093/mnras/stab608 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1093/mnras/stab608 (徳島大学機関リポジトリ: 116823, DOI: 10.1093/mnras/stab608)
16.	D. Arzoumanian, Ray S. Furuya, T. Hasegawa, M. Tahani, S. Sadavoy, H. C. L. Hull, D. Johnstone, M. P. Koch, S. Inutsuka, Y. Doi, T. Hoang, T. Onaka, K. Iwasaki, Y. Shimajiri, T. Inoue, N. Peretto, P. André, P. Bastien, D. Berry, V. H. -R. Chen, J. Francesco Di, C. Eswaraiah, L. Fanciullo, M. L. Fissel, J. Hwang, -h. J. Kang, G. Kim, -T. K. Kim, F. Kirchschlager, W. Kwon, W. C. Lee, -L. H. Liu, -R. A. Lyo, K. Pattle, A. Soam, X. Tang, A. Whitworth, -C. T. Ching, S. Coudé, -W. J. Wang, D. Ward-Thompson, -P. S. Lai, K. Qiu, L. T. Bourke, -Y. D. Byun, M. Chen, Z. Chen, P. W. Chen, J. Cho, Y. Choi and 99 more : Dust polarized emission observations of NGC 6334. BISTRO reveals the details of the complex but organized magnetic field structure of the high-mass star-forming hub-filament network, Astronomy & Astrophysics, Vol.647, A78, 2021. (出版サイトへのリンク) ● Publication site (DOI): 10.1051/0004-6361/202038624 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85102476715 (DOI: 10.1051/0004-6361/202038624, Elsevier: Scopus)
17.	Kate Pattle, Shih-Ping Lai, James Francesco Di, Sarah Sadavoy, Derek Ward-Thompson, Doug Johnstone, Thiem Hoang, Doris Arzoumanian, Pierre Bastien, L. Tyler Bourke, Simon Coudé, Yasuo Doi, Chakali Eswaraiah, Lapo Fanciullo, Ray S. Furuya, Jihye Hwang, H. Charles L. Hull, Jihyun Kang, Kee-Tae Kim, Florian Kirchschlager, Jungmi Kwon, Woojin Kwon, Won Chang Lee, Tie Liu, Matt Redman, Archana Soam, Mehrnoosh Tahani, Motohide Tamura and Xindi Tang : JCMT POL-2 and BISTRO Survey Observations of Magnetic Fields in the L1689 Molecular Cloud, The Astrophysical Journal, Vol.907, No.2, 88, 2021. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/abcc6c (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.3847/1538-4357/abcc6c (DOI: 10.3847/1538-4357/abcc6c)
18.	Bich Nguyen Ngoc, Ngoc Pham Diep, Harriet Parsons, Kate Pattle, Thiem Hoang, Derek Ward-Thompson, Ngoc Le Tram, H. Charles L. Hull, Mehrnoosh Tahani, Ray S. Furuya, Pierre Bastien, Keping Qiu, Tetsuo Hasegawa, Woojin Kwon, Yasuo Doi, Shih-Ping Lai, Simon Coudé, David Berry, Tao-Chung Ching, Jihye Hwang, Archana Soam, Jia-Wei Wang, Doris Arzoumanian, L. Tyler Bourke, Do-Young Byun, Vivien Huei-Ru Chen, Zhiwei Chen, Ping Wen Chen, Mike Chen, Jungyeon Cho, Yunhee Choi, Minho Choi, Antonio Chrysostomou, Jung Eun Chung, Sophia Dai, James Francesco Di, Yan Duan, Hao-Yuan Duan, David Eden, Chakali Eswaraiah, Lapo Fanciullo, Jason Fiege, M. Laura Fissel, Erica Franzmann, Per Friberg, Rachel Friesen, Gary Fuller, Tim Gledhill, Sarah Graves, Jane Greaves and 99 more : Observations of Magnetic Fields Surrounding LkHα 101 Taken by the BISTRO Survey with JCMT-POL-2, The Astrophysical Journal, Vol.908, No.1, 10, 2021. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/abd0fc (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85101515721 (DOI: 10.3847/1538-4357/abd0fc, Elsevier: Scopus)
19.	Hsi-Wei Yen, M. Patrick Koch, H. Charles L. Hull, Derek Ward-Thompson, Pierre Bastien, Tetsuo Hasegawa, Woojin Kwon, Shih-Ping Lai, Keping Qiu, Tao-Chung Ching, Jung Eun Chung, Simon Coudé, James Francesco Di, Ngoc Pham Diep, Yasuo Doi, Chakali Eswaraiah, Sam Falle, Gary Fuller, Ray S. Furuya, Jennifer Ilseung Hatchell Han, Martin Houde, Shu-ichiro Inutsuka, Doug Johnstone, Ji-hyun Kang, Miju Kang, Kee-Tae Kim, Florian Kirchschlager, Jungmi Kwon, Won Chang Lee, Chin-Fei Lee, Hong-Li Liu, Tie Liu, -Ran A. Lyo, Nagayoshi Ohashi, Takashi Onaka, Kate Pattle, Sarah Sadavoy, Hiro Saito, Hiroko Shinnaga, Archana Soam, Mehrnoosh Tahani, Motohide Tamura, Ya-Wen Tang, Xindi Tang and Chuan-Peng Zhang : The JCMT BISTRO Survey: Alignment between Outflows and Magnetic Fields in Dense Cores/Clumps, The Astrophysical Journal, Vol.907, No.1, 33, 2021. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/abca99 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85100837788 (DOI: 10.3847/1538-4357/abca99, Elsevier: Scopus)
20.	Yasuo Doi, Tetsuo Hasegawa, Ray S. Furuya and more 135 and : The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333, The Astrophysical Journal, Vol.899, No.id.28, 1-33, 2020. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/aba1e2 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.3847/1538-4357/aba1e2 (DOI: 10.3847/1538-4357/aba1e2)
21.	Axel Brandenburg and Ray S. Furuya : Application of a helicity proxy to edge-on galaxies, Monthly Notices of the Royal Astronomical Society, Vol.496, No.4, 4749-4759, 2020. (徳島大学機関リポジトリ) ● Metadata: 116243 (出版サイトへのリンク) ● Publication site (DOI): 10.1093/mnras/staa1795 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1093/mnras/staa1795 (徳島大学機関リポジトリ: 116243, DOI: 10.1093/mnras/staa1795)
22.	Ward-Thompson Derek, F. Christopher McKee, Ray S. Furuya and Yusuke Tsukamoto : Editorial: The Role of Magnetic Fields in the Formation of Stars, Frontiers in Astronomy and Space Sciences, Vol.7, No.13, 2020. (徳島大学機関リポジトリ) ● Metadata: 115260 (出版サイトへのリンク) ● Publication site (DOI): 10.3389/fspas.2020.00013 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.3389/fspas.2020.00013 (徳島大学機関リポジトリ: 115260, DOI: 10.3389/fspas.2020.00013)
23.	Kate Pattle, Ray S. Furuya and al. et : JCMT BISTRO Survey Observations of the Ophiuchus Molecular Cloud: Dust Grain Alignment Properties Inferred Using a Ricean Noise Model, The Astrophysical Journal, Vol.880, No.1, articleid.27-16pp, 2019. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/ab286f (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.3847/1538-4357/ab286f (DOI: 10.3847/1538-4357/ab286f)
24.	Simon Coudé, Ray S. Furuya and al. et : The JCMT BISTRO Survey: The Magnetic Field of the Barnard 1 Star-forming Region, The Astrophysical Journal, Vol.877, No.2, articleid.8817pp, 2019. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/ab1b23 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.3847/1538-4357/ab1b23 (DOI: 10.3847/1538-4357/ab1b23)
25.	Jia-Wei Wang, Ray S. Furuya and al. et : JCMT BISTRO Survey: Magnetic Fields within the Hub-filament Structure in IC 5146, The Astrophysical Journal, Vol.876, No.1, articleid.42-19pp, 2019. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/ab13a2 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.3847/1538-4357/ab13a2 (DOI: 10.3847/1538-4357/ab13a2)
26.	Junhao Liu, Ray S. Furuya and al. et : The JCMT BISTRO Survey: The Magnetic Field in the Starless Core ρ Ophiuchus C, The Astrophysical Journal, Vol.877, No.1, articleid.43-17pp, 2019. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/ab0958 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.3847/1538-4357/ab0958 (DOI: 10.3847/1538-4357/ab0958)
27.	Ray S. Furuya, Kitamura Yoshimi and Shinnaga Hiroko : A 1000 au Scale Molecular Outflow Driven by a Protostar with an Age of <4000 yr, The Astrophysical Journal, Vol.871, No.2, articleid.137-19pages, 2019. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/aaf85c (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.3847/1538-4357/aaf85c (DOI: 10.3847/1538-4357/aaf85c)
28.	Archana Soam, Kate Pattle, Derek Ward-Thompson, Chang Won Lee, Sarah Sadavoy, Patrick M. Koch, Gwanjeong Kim, Jungmi Kwon, Woojin Kwon, Doris Arzoumanian, David Berry, Thiem Hoang, Motohide Tamura, Sang-Sung Lee, Tie Liu, Kee-Tae Kim, Doug Johnstone, Fumitaka Nakamura, A-Ran Lyo, Takashi Onaka, Jongsoo Kim, Ray S. Furuya, Tetsuo Hasegawa, Shih-Ping Lai, Pierre Bastien, Eun Jung Chung, Shinyoung Kim, Harriet Parsons, Mark Rawlings, Mairs Steve and et al. : Magnetic fields towards Ophiuchus-B derived from SCUBA-2 polarization measurements, The Astrophysical Journal, Vol.861, No.1, articleid.65-13pp, 2018. (要約) We present the results of dust emission polarization measurements of Ophiuchus-B (Oph-B) carried out using the Submillimetre Common-User Bolometer Array 2 (SCUBA-2) camera with its associated polarimeter (POL-2) on the James Clerk Maxwell Telescope (JCMT) in Hawaii. This work is part of the B-fields In Star-forming Region Observations (BISTRO) survey initiated to understand the role of magnetic fields in star formation for nearby star-forming molecular clouds. We present a first look at the geometry and strength of magnetic fields in Oph-B. The field geometry is traced over 0.2 pc, with clear detection of both of the sub-clumps of Oph-B. The field pattern appears significantly disordered in sub-clump Oph-B1. The field geometry in Oph-B2 is more ordered, with a tendency to be along the major axis of the clump, parallel to the filamentary structure within which it lies. The degree of polarization decreases systematically towards the dense core material in the two sub-clumps. The field lines in the lower density material along the periphery are smoothly joined to the large scale magnetic fields probed by NIR polarization observations. We estimated a magnetic field strength of 630±410 G in the Oph-B2 sub-clump using a Davis-Chandeasekhar-Fermi analysis. With this magnetic field strength, we find a mass-to-flux ratio = 1.6±1.1, which suggests that the Oph-B2 clump is slightly magnetically supercritical. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/aac4a6 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.3847/1538-4357/aac4a6 (DOI: 10.3847/1538-4357/aac4a6)
29.	Kate Pattle, Derek Ward-Thompson, Tetsuo Hasegawa, Pierre Bastien, Woojin Kwon, Shih-Ping Lai, Keping Qiu, Ray S. Furuya, David Berry and The JCMT BISTRO Survey Team : First Observations of the Magnetic Field inside the Pillars of Creation: Results from the BISTRO Survey, The Astrophysical Journal Letters, Vol.860, No.1, 2018. (要約) We present the first high-resolution, submillimeter-wavelength polarimetric observations of and thus direct observations of the magnetic field morphology within the dense gas of the Pillars of Creation in M16. These 850 m observations, taken as part of the B-Fields in Star-forming Region Observations Survey (BISTRO) using the POL-2 polarimeter on the Submillimeter Common-User Bolometer Array 2 (SCUBA-2) camera on the James Clerk Maxwell Telescope (JCMT), show that the magnetic field runs along the length of the Pillars, perpendicular to and decoupled from the field in the surrounding photoionized cloud. Using the Chandrasekhar Fermi method we estimate a plane-of-sky magnetic field strength of 170 320 G in the Pillars, consistent with their having been formed through the compression of gas with initially weak magnetization. The observed magnetic field strength and morphology suggests that the magnetic field may be slowing the Pillars' evolution into cometary globules. We thus hypothesize that the evolution and lifetime of the Pillars may be strongly influenced by the strength of the coupling of their magnetic field to that of their parent photoionized cloud i.e., that the Pillars' longevity results from magnetic support. (徳島大学機関リポジトリ) ● Metadata: 115006 (出版サイトへのリンク) ● Publication site (DOI): 10.3847/2041-8213/aac771 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85049008563 (徳島大学機関リポジトリ: 115006, DOI: 10.3847/2041-8213/aac771, Elsevier: Scopus)
30.	Jungmi Kwon, Yasuo Doi, Motohide Tamura, Masafumi Matsumura, Kate Pattle, David Berry, Sarah Sadavoy, Brenda C. Matthews, Derek Ward-Thompson, Tetsuo Hasegawa, Ray S. Furuya and et al. : A First Look at BISTRO Observations of the ϱ Oph-A core, The Astrophysical Journal, Vol.859, No.1, 2018. (要約) We present 850 m imaging polarimetry data of the Oph-A core taken with the Submillimeter Common-User Bolometer Array-2 (SCUBA-2) and its polarimeter (POL-2) as part of our ongoing survey project, ${oldsymbol{B}}$-fields In STar forming RegiOns (BISTRO). The polarization vectors are used to identify the orientation of the magnetic field projected on the plane of the sky at a resolution of 0.01 pc. We identify 10 subregions with distinct polarization fractions and angles in the 0.2 pc Oph-A core; some of them can be part of a coherent magnetic field structure in the Oph region. The results are consistent with previous observations of the brightest regions of Oph-A, where the degrees of polarization are at a level of a few percent, but our data reveal for the first time the magnetic field structures in the fainter regions surrounding the core where the degree of polarization is much higher (>5%). A comparison with previous near-infrared polarimetric data shows that there are several magnetic field components that are consistent at near-infrared and submillimeter wavelengths. Using the Davis Chandrasekhar Fermi method, we also derive magnetic field strengths in several subcore regions, which range from approximately 0.2 to 5 mG. We also find a correlation between the magnetic field orientations projected on the sky and the core centroid velocity components. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/aabd82 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85047882276 (DOI: 10.3847/1538-4357/aabd82, Elsevier: Scopus)
31.	Kate Pattle, Derek Ward-Thompson, David Berry, Jennifer Hatchell, Huei-Ru Chen, Andy Pon, Patrick M. Koch, Woojin Kwon, Jongsoo Kim, Pierre Bastien, Jungyeon Cho, Simon Coudé, James Di Francesco, Gary Fuller, Ray S. Furuya, Sarah F. Graves, Doug Johnstone, Jason Kirk, Jungmi Kwon, Chang Won Lee, Brenda C. Matthews, Joseph C. Mottram, Harriet Parsons, Sarah Sadavoy, Hiroko Shinnaga, Archana Soam, Tetsuo Hasegawa, Shih-Ping Lai, Keping Qiu and Per Friberg : The JCMT BISTRO Survey: The Magnetic Field Strength in the Orion A Filament, The Astrophysical Journal, Vol.846, No.2, 2017. (要約) We determine the magnetic field strength in the OMC 1 region of the Orion A filament via a new implementation of the Chandrasekhar Fermi method using observations performed as part of the James Clerk Maxwell Telescope (JCMT) B-Fields In Star-forming Region Observations (BISTRO) survey with the POL-2 instrument. We combine BISTRO data with archival SCUBA-2 and HARP observations to find a plane-of-sky magnetic field strength in OMC 1 of ${B}_{athrm{pos}}=6.6m 4.7$ mG, where $elta {B}_{athrm{pos}}=4.7$ mG represents a predominantly systematic uncertainty. We develop a new method for measuring angular dispersion, analogous to unsharp masking. We find a magnetic energy density of $im 1.7imes {10}^{-7}$ J m-3 in OMC 1, comparable both to the gravitational potential energy density of OMC 1 (~10-7 J m-3) and to the energy density in the Orion BN/KL outflow (~10-7 J m-3). We find that neither the Alfvén velocity in OMC 1 nor the velocity of the super-Alfvénic outflow ejecta is sufficiently large for the BN/KL outflow to have caused large-scale distortion of the local magnetic field in the ~500 yr lifetime of the outflow. Hence, we propose that the hourglass field morphology in OMC 1 is caused by the distortion of a primordial cylindrically symmetric magnetic field by the gravitational fragmentation of the filament and/or the gravitational interaction of the BN/KL and S clumps. We find that OMC 1 is currently in or near magnetically supported equilibrium, and that the current large-scale morphology of the BN/KL outflow is regulated by the geometry of the magnetic field in OMC 1, and not vice versa. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/aa80e5 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85029528706 (DOI: 10.3847/1538-4357/aa80e5, Elsevier: Scopus)
32.	P. Hofner, R. Cesaroni, S. Kurtz, V. Rosero, C. Anderson, Ray S. Furuya, E. D. Araya and S. Molinari : High-resolution Observations of the Massive Protostar in IRAS 18566+0408, The Astrophysical Journal, Vol.843, No.2, 2017. (要約) We report 3 mm continuum, CH3CN(5 4) and 13CS(2 1) line observations with CARMA (Combined Array for Research in Millimeter-wave Astronomy), in conjunction with 6 and 1.3 cm continuum VLA data, and 12 and 25 m broadband data from the Subaru Telescope toward the massive proto-star IRAS 18566+0408. The VLA data resolve the ionized jet into four components aligned in the E W direction. Radio components A, C, and D have flat centimeter SEDs indicative of optically thin emission from ionized gas, and component B has a spectral index = 1.0, and a decreasing size with frequency $ropto {u }^{-0.5}$. Emission from the CARMA 3 mm continuum and from the 13CS(2 1) and CH3CN(5 4) spectral lines is compact (i.e., $t 6700athrm{au}$) and peaks near the position of the VLA centimeter source, component B. Analysis of these lines indicates hot and dense molecular gas, which is typical for HMCs. Our Subaru telescope observations detect a single compact source, coincident with radio component B, demonstrating that most of the energy in IRAS 18566+0408 originates from a region of size $t 2400athrm{au}$. We also present UKIRT near-infrared archival data for IRAS 18566+0408, which show extended K-band emission along the jet direction. We detect an E W velocity shift of about 10 km s-1 over the HMC in the CH3CN lines possibly tracing the interface of the ionized jet with the surrounding core gas. Our data demonstrate the presence of an ionized jet at the base of the molecular outflow and support the hypothesis that massive protostars with O-type luminosity form with a mechanism similar to lower mass stars. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/aa7459 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85025122845 (DOI: 10.3847/1538-4357/aa7459, Elsevier: Scopus)
33.	Derek Ward-Thompson, Kate Pattle, Pierre Bastien, Ray S. Furuya, Woojin Kwon, Shih-Ping Lai, Keping Qiu, David Berry, Minho Choi, Simon Coudé and et al. : First Results from BISTRO: A SCUBA-2 Polarimeter Survey of the Gould Belt, The Astrophysical Journal, Vol.842, No.1, 2017. (要約) We present the first results from the B-fields In STar-forming Region Observations (BISTRO) survey, using the Sub-millimetre Common-User Bolometer Array 2 camera, with its associated polarimeter (POL-2), on the James Clerk Maxwell Telescope in Hawaii. We discuss the survey's aims and objectives. We describe the rationale behind the survey, and the questions that the survey will aim to answer. The most important of these is the role of magnetic fields in the star formation process on the scale of individual filaments and cores in dense regions. We describe the data acquisition and reduction processes for POL-2, demonstrating both repeatability and consistency with previous data. We present a first-look analysis of the first results from the BISTRO survey in the OMC 1 region. We see that the magnetic field lies approximately perpendicular to the famous "integral filament" in the densest regions of that filament. Furthermore, we see an "hourglass" magnetic field morphology extending beyond the densest region of the integral filament into the less-dense surrounding material, and discuss possible causes for this. We also discuss the more complex morphology seen along the Orion Bar region. We examine the morphology of the field along the lower-density northeastern filament. We find consistency with previous theoretical models that predict magnetic fields lying parallel to low-density, non-self-gravitating filaments, and perpendicular to higher-density, self-gravitating filaments. (出版サイトへのリンク) ● Publication site (DOI): 10.3847/1538-4357/aa70a0 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-85021147408 (DOI: 10.3847/1538-4357/aa70a0, Elsevier: Scopus)
34.	Ray S. Furuya and Yoshiaki Taniguchi : A massive dense gas cloud close to the nucleus of the Seyfert galaxy NGC 1068, Publications of the Astronomical Society of Japan, Vol.68, No.6, 2016. (要約) Using the ALMA archival data of both 12CO (6 5) line and 689-GHz continuum emission towards the archetypical Seyfert galaxy, NGC 1068, we identified a distinct continuum peak separated by 15 pc from the nuclear radio component S1 in projection. The continuum flux gives a gas mass of 2 × 105 M and bolometric luminosity of 108 L, leading to a star formation rate of 0.1 M yr-1. Subsequent analysis on the line data suggest that the gas cloud has a size of 10 pc, yielding to a mean H2 number density of 105 cm-3. We therefore refer to the gas as a ''massive dense gas cloud'': the gas density is high enough to form a ''protostar cluster'' with a stellar mass of 104 M. We found that the gas stands at a unique position between galactic and extraglactic clouds in the diagrams of start formation rate (SFR) vs. gas mass proposed by Lada et al. (2012, ApJ, 745, 190) and surface density of gas vs. SFR density by Krumholz and McKee (2005, ApJ, 630, 250). All the gaseous and star-formation properties may be understood in terms of the turbulence-regulated star formation scenario. Since there are two stellar populations with ages of 300 Myr and 30 Myr in the 100 pc scale circumnulear region, we discuss that NGC 1068 has experienced at least three episodic star-formation events with the likelihood that the inner star-forming region is the younger. Together with several lines of evidence that the dynamics of the nuclear region is decoupled from that of the entire galactic disk, we discuss that the gas inflow towards the nuclear region of NGC 1068 may be driven by a past minor merger. (出版サイトへのリンク) ● Publication site (DOI): 10.1093/pasj/psw095 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1093/pasj/psw095 (DOI: 10.1093/pasj/psw095)
35.	T. M. Beltrán, Á. Sánchez-Monge, R. Cesaroni, M. N. S. Kumar, D. Galli, C. M. Walmsley, S. Etoka, Ray S. Furuya, L. Moscadelli, T. Stanke, F. der van S. F. Tak, S. Vig, K.-S. Wang, H. Zinnecker, D. Elia and E. Schisano : Filamentary structure and Keplerian rotation in the high-mass star-forming region G35.03+0.35 imaged with ALMA, Astronomy & Astrophysics, Vol.571, No.article id. A52, 24-pages, 2014. (出版サイトへのリンク) ● Publication site (DOI): 10.1051/0004-6361/201424031 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1051/0004-6361/201424031 (DOI: 10.1051/0004-6361/201424031)
36.	Ray S. Furuya, Kitamura Yoshimi and Shinnaga Hiroko : A Dynamically Collapsing Core and a Precursor of a Core in a Filament Supported by Turbulent and Magnetic Pressures, The Astrophysical Journal, Vol.793, No.article id.94, 23-pages, 2014. (出版サイトへのリンク) ● Publication site (DOI): 10.1088/0004-637X/793/2/94 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1088/0004-637X/793/2/94 (DOI: 10.1088/0004-637X/793/2/94)
37.	L. Moscadelli, R. Cesaroni, Á. Sánchez-Monge, C. Goddi, Ray S. Furuya, A. Sanna and M. Pestalozzi : A study on subarcsecond scales of the ammonia and continuum emission toward the G16.59-0.05 high-mass star-forming region, Astronomy & Astrophysics, Vol.558, No.A145, 11, 2013. (要約) Aims. We wish to investigate the structure, velocity field, and stellar content of the G16.590.05 high-mass star-forming region, where previous studies have established the presence of two almost perpendicular (NESW and SENW), massive outflows, and a rotating disk traced by methanol maser emission.Methods. We performed Very Large Array observations of the radio continuum and ammonia line emission, complemented by COMICS/Subaru and Hi-GAL/Herschel images in the mid- and far-infrared.Results. Our centimeter continuum maps reveal a collimated radio jet that is oriented EW and centered on the methanol maser disk, placed at the SE border of a compact molecular core. The spectral index of the jet is negative, indicating non-thermal emission over most of the jet, except the peak close to the maser disk, where thermal free-free emission is observed. We find that the ammonia emission presents a bipolar structure consistent (on a smaller scale) in direction and velocity with that of the NESW bipolar outflow detected in previous CO observations. After analyzing our previous N2H+(10) observations again, we conclude that two scenarios are possible. In one case both the radio jet and the ammonia emission would trace the root of the large-scale CO bipolar outflow. The different orientation of the jet and the ammonia flow could be explained by precession and/or a non-isotropic density distribution around the star. In the other case, the N2H+(10) and ammonia bipolarity is interpreted as two overlapping clumps moving with different velocities along the line of sight. The ammonia gas also seems to undergo rotation consistent with the maser disk. Our infrared images complemented by archival data allow us to derive a bolometric luminosity of ~104 L and to conclude that most of the luminosity is due to the young stellar object associated with the maser disk.Conclusions. The new data suggest a scenario where the luminosity and the outflow activity of the whole region could be dominated by two massive young stellar objects: 1) a B-type star of ~12 M at the center of the maser/ammonia disk; 2) a massive young stellar object (so far undetected), very likely in an earlier stage of evolution than the B-type star, which might be embedded inside the compact molecular core and power the massive, SENW outflow. (出版サイトへのリンク) ● Publication site (DOI): 10.1051/0004-6361/201321951 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1051/0004-6361/201321951 (DOI: 10.1051/0004-6361/201321951)
38.	J. J. Li, L. Moscadelli, R. Cesaroni, Ray S. Furuya, Y. Xu, T. Usuda, M. K. Menten, M. Pestalozzi, D. Elia and E. Schisano : Massive star-formation toward G28.87+0.07 (IRAS 18411 0338) investigated by means of maser kinematics and radio to infrared, continuum observations, The Astrophysical Journal, Vol.749, No.47, 16pages, 2012. (出版サイトへのリンク) ● Publication site (DOI): 10.1088/0004-637X/749/1/47 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1088/0004-637X/749/1/47 (DOI: 10.1088/0004-637X/749/1/47)
39.	Ray S. Furuya, R. Cesaroni and H Shinnaga : Infall, outflow, and rotation in the G19.61- 0.23 hot molecular core, Astronomy & Astrophysics, Vol.525, No.A72, 18pages, 2011. (出版サイトへのリンク) ● Publication site (DOI): 10.1051/0004-6361/201014402 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1051/0004-6361/201014402 (DOI: 10.1051/0004-6361/201014402)
40.	F. Fontani, R. Cesaroni and Ray S. Furuya : Class I and Class II methanol masers in high-mass star forming regions, Astronomy & Astrophysics, Vol.517, No.A56, 24pages, 2010. (出版サイトへのリンク) ● Publication site (DOI): 10.1051/0004-6361/200913679 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1051/0004-6361/200913679 (DOI: 10.1051/0004-6361/200913679)
41.	A. Sanna, L. Moscadelli, R. Cesaroni, A. Tarchi, Ray S. Furuya and C. Goddi : VLBI study of maser kinematics in high-mass SFRs. I. G16.59-0.05, Astronomy & Astrophysics, Vol.517, No.A71, 15pages, 2010. (出版サイトへのリンク) ● Publication site (DOI): 10.1051/0004-6361/201014233 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1051/0004-6361/201014233 (DOI: 10.1051/0004-6361/201014233)
42.	A. Sanna, L. Moscadelli, R. Cesaroni, A. Tarchi, Ray S. Furuya and C. Goddi : VLBI study of maser kinematics in high-mass SFRs. II. G23.01-0.41, Astronomy & Astrophysics, Vol.517, No.A78, 19pages, 2010. (出版サイトへのリンク) ● Publication site (DOI): 10.1051/0004-6361/201014234 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1051/0004-6361/201014234 (DOI: 10.1051/0004-6361/201014234)
43.	C. Codella, R. Cesaroni, A. López-Sepulcre, M. T. Beltrán, Ray S. Furuya and L. Testi : Looking for high-mass young stellar objects: and H₂O masers in massive ammonia cores, Astronomy & Astrophysics, Vol.510, No.A86, 16pages, 2010. (出版サイトへのリンク) ● Publication site (DOI): 10.1051/0004-6361/200913371 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1051/0004-6361/200913371 (DOI: 10.1051/0004-6361/200913371)
44.	Hiroko Shinnaga, G. Thomas Phillips, Ray S. Furuya and Yoshimi Kitamura : Warm Extended Dense Gas Lurking At The Heart of A Cold Collapsing Dense Core, The Astrophysical Journal Letters, Vol.706, No.2, L226-L229, 2009. (出版サイトへのリンク) ● Publication site (DOI): 10.1088/0004-637X/706/2/L226 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1088/0004-637X/706/2/L226 (DOI: 10.1088/0004-637X/706/2/L226)
45.	Ray S. Furuya and Hiroko Shinnaga : High Velocity Outflow in CO J=7 6 from the Orion Hot Core, The Astrophysical Journal, Vol.703, No.2, 1198-1202, 2009. (出版サイトへのリンク) ● Publication site (DOI): 10.1088/0004-637X/703/2/1198 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1088/0004-637X/703/2/1198 (DOI: 10.1088/0004-637X/703/2/1198)
46.	Ray S. Furuya, Yoshimi Kitamura and Hiroko Shinnaga : Spectroscopic Evidence for Gas Infall in GF9-2, The Astrophysical Journal Letters, Vol.692, No.2, L96-L99, 2009. (出版サイトへのリンク) ● Publication site (DOI): 10.1088/0004-637X/692/2/L96 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1088/0004-637X/692/2/L96 (DOI: 10.1088/0004-637X/692/2/L96)
47.	Hiroko Shinnaga, G. Thomas Phillips, Ray S. Furuya and Riccardo Cesaroni : Submillimeter Observations of the Isolated Massive Dense Clump IRAS 20126+4104, The Astrophysical Journal, Vol.682, No.2, 1103-1113, 2008. (出版サイトへのリンク) ● Publication site (DOI): 10.1086/589279 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1086/589279 (DOI: 10.1086/589279)
48.	Ray S. Furuya, Yoshimi Kitamura and Hiroko Shinnaga : Low-Mass Star-Forming Cores in the GF9 Filament, Publications of the Astronomical Society of Japan, Vol.60, No.3, 421-428, 2008. (キーワード) ISM : clouds / ISM : evolution / ISM : individual (GF9, L1082) / ISM : molecules / stars : formation / stars : pre-main sequence (文献検索サイトへのリンク) ● CiNii @ 国立情報学研究所 (CRID): 1520010380831674112 ● Summary page in Scopus @ Elsevier: 2-s2.0-48249136164 (CiNii: 1520010380831674112, Elsevier: Scopus)
49.	Ray S. Furuya, R. Cesaroni, S. Takahashi, C. Codella, M. Momose and M. T. Beltrán : Candidate Rotating Toroids around High-Mass (Proto)Stars, The Astrophysical Journal, Vol.673, No.1, 363-381, 2008. (出版サイトへのリンク) ● Publication site (DOI): 10.1086/523834 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1086/523834 (DOI: 10.1086/523834)
50.	L. Moscadelli, C. Goddi, R. Cesaroni, M. T. Beltrán and Ray S. Furuya : Massive Star- Formation in G24.78+0.08 Explored through VLBI Maser Observations, Astronomy & Astrophysics, Vol.472, No.3, 867-879, 2007. (出版サイトへのリンク) ● Publication site (DOI): 10.1051/0004-6361:20077823 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1051/0004-6361:20077823 (DOI: 10.1051/0004-6361:20077823)
51.	Ray S. Furuya, Yoshimi Kitamura and Hiroko Shinnaga : The Initial Conditions for Gravitational Collapse of a Core: An Extremely Young Low-Mass Class 0 Protostar GF9-2, The Astrophysical Journal, Vol.653, No.2, 1369-1390, 2006. (出版サイトへのリンク) ● Publication site (DOI): 10.1086/508405 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1086/508405 (DOI: 10.1086/508405)
52.	Maria T. Beltrán, Riccardo Cesaroni, Claudio Codella, Leonardo Testi, Ray S. Furuya and Luca Olmi : Infall of Gas as the Formation Mechanism of Stars with Mass up to 20 Times More Massive than the Sun, Nature, Vol.443, No.7110, 427-429, 2006. (要約) Theory predicts and observations confirm that low-mass stars (like the Sun) in their early life grow by accreting gas from the surrounding material. But for stars approximately 10 times more massive than the Sun (approximately 10M(o)), the powerful stellar radiation is expected to inhibit accretion and thus limit the growth of their mass. Clearly, stars with masses >10M(o) exist, so there must be a way for them to form. The problem may be solved by non-spherical accretion, which allows some of the stellar photons to escape along the symmetry axis where the density is lower. The recent detection of rotating disks and toroids around very young massive stars has lent support to the idea that high-mass ( > 8M(o)) stars could form in this way. Here we report observations of an ammonia line towards a high-mass star forming region. We conclude that the gas is falling inwards towards a very young star of approximately 20M(o), in line with theoretical predictions of non-spherical accretion. (出版サイトへのリンク) ● Publication site (DOI): 10.1038/nature05074 (文献検索サイトへのリンク) ● PubMed @ National Institutes of Health, US National Library of Medicine (PMID): 17006508 ● Search Scopus @ Elsevier (PMID): 17006508 ● Search Scopus @ Elsevier (DOI): 10.1038/nature05074 (DOI: 10.1038/nature05074, PubMed: 17006508)
53.	L. Moscadelli, L. Testi, Ray S. Furuya, G. Goddi, M. Claussen, Y. Kitamura and A. Wootten : First results from a VLBA Proper Motion Survey of H₂O Masers in Low-Mass YSOs: the Serpens Core and RNO15-FIR, Astronomy & Astrophysics, Vol.446, No.3, 985-999, 2006. (出版サイトへのリンク) ● Publication site (DOI): 10.1051/0004-6361:20053610 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1051/0004-6361:20053610 (DOI: 10.1051/0004-6361:20053610)
54.	Maria T. Beltrán, Riccardo Cesaroni, Roberto Neri, Claudio Codella, Ray S. Furuya, Leonardo Testi and Luca Olmi : A Detailed Study of the Rotating toroids in G31.41+0.31 and G24.78+0.08, Astronomy & Astrophysics, Vol.435, No.3, 901-925, 2005. (出版サイトへのリンク) ● Publication site (DOI): 10.1051/0004-6361:20042381 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1051/0004-6361:20042381 (DOI: 10.1051/0004-6361:20042381)
55.	Ray S. Furuya, R. Cesaroni, S. Takahashi, M. Momose, L. Testi, H. Shinnaga and C. Codella : Relative Evolutionary Time Scale of Hot Molecular Cores with Respect to Ultra Compact HII Regions, The Astrophysical Journal, Vol.624, No.2, 827-831, 2005. (出版サイトへのリンク) ● Publication site (DOI): 10.1086/429286 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1086/429286 (DOI: 10.1086/429286)
56.	Ray S. Furuya, Yoshimi Kitamura, Alwyn Wootten, Mark J. Claussen and Ryohei Kawabe : Proper Motion of H₂O Masers in IRAS 20050+2720 MMS1: An AU Scale Jet Associated with An Intermediate- Mass Class 0 Source, Astronomy & Astrophysics, Vol.438, No.2, 571-583, 2005. (出版サイトへのリンク) ● Publication site (DOI): 10.1051/0004-6361:20034189 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1051/0004-6361:20034189 (DOI: 10.1051/0004-6361:20034189)
57.	Maria T. Beltrán, Riccardo Cesaroni, Roberto Neri, C. Codella, Ray S. Furuya, Leonardo Testi and Luca Olmi : Rotating Disks in High-Mass Young Stellar Objects, The Astrophysical Journal, Vol.601, No.2, L187-L190, 2004. (出版サイトへのリンク) ● Publication site (DOI): 10.1086/382150 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-1842533073 (DOI: 10.1086/382150, Elsevier: Scopus)
58.	Ray S. Furuya, Hiroko Shinnaga, Kouichiro Nakanishi, Munetake Momose and Masao Saito : A Giant Flare on a T Tauri Star Observed at Millimeter Wavelengths, Publications of the Astronomical Society of Japan, Vol.55, No.6, L83-L87, 2003. (キーワード) radio continuum : stars / stars : flare / stars : individual (GMR-A) / stars : pre-main-sequence / techniques : interferometric (文献検索サイトへのリンク) ● CiNii @ 国立情報学研究所 (CRID): 1520573329775466880 ● Summary page in Scopus @ Elsevier: 2-s2.0-1442352578 (CiNii: 1520573329775466880, Elsevier: Scopus)
59.	Ray S. Furuya, M. C. Walmsley, K. Nakanishi, P. Schilke and R. Bachiller : Interferometric Observations of FeO towards Sagittarius B2, Astronomy & Astrophysics, Vol.409, No.2, L21-L24, 2003. (出版サイトへのリンク) ● Publication site (DOI): 10.1051/0004-6361:20031304 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1051/0004-6361:20031304 (DOI: 10.1051/0004-6361:20031304)
60.	R. Cesaroni, C. Codella, Ray S. Furuya and L. Testi : Anatomy of a High-Mass Star Forming Cloud: The G24.78+0.08 (Proto)Stellar Cluster, Astronomy & Astrophysics, Vol.401, No.1, 227-242, 2003. (出版サイトへのリンク) ● Publication site (DOI): 10.1051/0004-6361:20030116 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-0037380647 (DOI: 10.1051/0004-6361:20030116, Elsevier: Scopus)
61.	Ray S. Furuya, Yoshimi Kitamura, Alwyn H. Wootten, J. Mark Claussen and Ryohei Kawabe : Water Maser Survey towards Low-Mass Young Stellar Objects in the Northern Sky with the Nobeyama 45-m Telescope and the Very Large Array, The Astrophysical Journal. Supplement Series, Vol.144, No.1, 71-134, 2003. (出版サイトへのリンク) ● Publication site (DOI): 10.1086/342749 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1086/342749 (DOI: 10.1086/342749)
62.	F. W. R. Dent, Ray S. Furuya and J. C. Davis : The Impact of HH2 on Local Dust and Gas, Monthly Notices of the Royal Astronomical Society, Vol.339, 633-640, 2003. (出版サイトへのリンク) ● Publication site (DOI): 10.1046/j.1365-8711.2003.06180.x (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1046/j.1365-8711.2003.06180.x (DOI: 10.1046/j.1365-8711.2003.06180.x)
63.	Ray S. Furuya, R. Cesaroni, L. Testi, C. Codella, R. Bachiller and M. Tafalla : G24.78 +0.08: A Cluster of High-Mass (Proto)Stars, Astronomy & Astrophysics, Vol.390, No.1, L1-L4, 2002. (出版サイトへのリンク) ● Publication site (DOI): 10.1051/0004-6361:20020850 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-0036647440 (DOI: 10.1051/0004-6361:20020850, Elsevier: Scopus)
64.	Ray S. Furuya, Yoshimi Kitamura, H. Alwyn Wootten, J. Mark Claussen and Ryohei Kawabe : Water Maser Survey toward Low-Mass Young Stellar Objects in the Northern Sky: Observational Constraints on Maser Excitation Conditions, The Astrophysical Journal Letters, Vol.559, No.2, L143-L147, 2001. (出版サイトへのリンク) ● Publication site (DOI): 10.1086/324012 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1086/324012 (DOI: 10.1086/324012)
65.	Ray S. Furuya, Yoshimi Kitamura, H. Alwyn Wootten, J. Mark Claussen, Masao Saito, B. Kevin Marvel and Ryohei Kawabe : A Microjet: A Protostar's Cry at Birth, The Astrophysical Journal, Vol.542, No.2, L135-L138, 2000. (出版サイトへのリンク) ● Publication site (DOI): 10.1086/312925 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-0034692753 (DOI: 10.1086/312925, Elsevier: Scopus)
66.	Ray S. Furuya, Yoshimi Kitamura, Masao Saito, Ryohei Kawabe and H. Alwyn Wootten : VLA Observations of H2O Masers in the Class 0 Protostar S106 FIR: Evidence for a 10 AU Scale Accelerating Jetlike Flow, The Astrophysical Journal, Vol.525, No.2, 821-831, 1999. (出版サイトへのリンク) ● Publication site (DOI): 10.1086/307913 (文献検索サイトへのリンク) ● Summary page in Scopus @ Elsevier: 2-s2.0-0033544233 (DOI: 10.1086/307913, Elsevier: Scopus)

学術論文(紀要・その他):

1.	Masafumi Matsumura, Ray S. Furuya, Tetsuo Hasegawa, Yasuo Doi and Koji S. Kawabata : Pinched Magnetic Field around the Massive Star Forming Region Monoceros R2: An Analysis of Planck Polarimetric Images, IAU Symposium No. 360, "Astronomical Polarimetry 2020: New Era of Multiwavelength Polarimetry", 2021.
2.	Sakiko Fukaya, Hiroko Shinnaga, Ray S. Furuya, Masahiro N. Machida and Kohji Tomisaka : Magnetic field of a dense core L1521 F in Taurus molecular cloud, IAU Symposium No. 360, "Astronomical Polarimetry 2020: New Era of Multiwavelength Polarimetry", 2021.
3.	Ray S. Furuya, Kate Pattle, Simon Coudé, Tao-Chung Ching and more Steve and 7 Mairs : Magnetic Fields Studies in the Next Decade: EAO Submillimetre Futures White Paper Series, 2019, EAO Submillimetre Futures White Paper Series, 2019, 1-17, 2020. (文献検索サイトへのリンク) ● CiNii @ 国立情報学研究所 (CRID): 1010568455821942658 (CiNii: 1010568455821942658)
4.	Ray S. Furuya, Yoshimi Kitamura and Hiroko Shinnaga : Compact Molecular Outflow from a Protostar at the Earliest Evolutionary Phase, "The Labyrinth of Star Formation", Astrophysics and Space Science Proceedings, Volume 36. ISBN 978-3-319-03040-1, Springer International Publishing Switzerland, Vol.36, 283-285, 2014. (出版サイトへのリンク) ● Publication site (DOI): 10.1007/978-3-319-03041-8_54 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.1007/978-3-319-03041-8_54 (DOI: 10.1007/978-3-319-03041-8_54)
5.	古屋 S. 玲, 齊藤隆仁, 荒木秀夫 : 徳島大学教員と徳島県内の高校関係者へのインタビュー調査, --- ―高校から大学への教育の接続をより良いものにするために― ---, 大学教育研究ジャーナル, Vol.10, No.10, 95-98, 2013年. (要約) これまで高等学校までの教育内容にゆとりを持たせていたことに加え,少子化による大学進学率の上昇が相まって,大学初年度で学ぶべき水準についていけない学生の存在が徳島大学においても顕在化している．一方で,大学卒業生の質は一定の水準を保つべきという社会的要請がある．この現状を鑑み,本学の理念に基づく,教育目標と教育水準を堅持するため,高校と大学の接続教育に求められるものは何かを明確にすることが求められている．このため,アンケート調査では拾い上げることが容易でない,教職員の率直な意見を2012年夏から冬にかけて大学と高校双方における対面インタビュー調査によって収集した．寄せられた意見と教育現場からの示唆の大部分は,中央教育審議会や日本学術会議等の答申等と整合する．したがって,大局的な見地に立ちつつ,地域の特性も考慮した,より良い高等教育システムを作り上げることが求められている． (キーワード) 高大接続 / 専門教育への接続 / 徳島大学 / 徳島県内高校 / 対面調査 (文献検索サイトへのリンク) ● CiNii @ 国立情報学研究所 (CRID): 1050564287418286464 (CiNii: 1050564287418286464)
6.	M. T. Beltrán, R. Cesaroni, L. Moscadelli, L Testi, C. Codella, Ray S. Furuya and C. Goddi : Infall and the Formation of a Massive Star, "Massive Star Formation: Observations Confront Theory", ASP Conference Series, Astronomical Society of the Pacific, Vol.387, 71-77, 2008.
7.	M. J. Claussen, H. A. Wootten, C. L. Brogan, K. B. Marvel and Ray S. Furuya : Probing Jet and Disk Winds toward Low-Mass Protostars, "Future Directions in High Resolution Astronomy: The 10th Anniversary of the VLBA", ASP Conference Proceedings, Astronomical Society of the Pacific, Vol.340, 324-328, 2005.
8.	Ray S. Furuya : H2O Masers in Young Stellar Objects, "Galactic Star Formation Across the Stellar Mass Spectrum", ASP Conference Series, Astronomical Society of the Pacific, Vol.287, 367-372, 2003.
9.	Ray S. Furuya, Y. Kitamura, A. Wootten, J. M. Claussen and R. Kawabe : Imaging of 2-mm dust continuum emission towards S106 FIR and its spectral energy distribution, "Cosmic Masers: From Proto-Stars to Black Holes", IAU Symposium 206, Astronomical Society of the Pacific, Vol.206, 22-25, 2002.

総説・解説:

1.	Doris Arzoumanian, 古屋 S. 玲 : 複雑で整然とした磁場構造:大質量星団を生み続ける最重量級ハブ・フィラメント, 天文月報, Vol.115, No.10, 631-642, 2022年10月.
2.	古屋 S. 玲 : 特集:物理科学, この1 年「サブミリ波偏波観測でみえた星形成ガスの磁場」, パリティ, Vol.34, No.1, 56-58, 2019年1月.

国際会議:

1.	Ray S. Furuya : Large Submillimeter Telescope: Science Goals and Technical Challenges, Union Radio-Scientifique Internationale, Japan National Committee 2022 Meeting, http://www.ursi.jp/conference/jrsm2022/, Tokyo, Japan, Sep. 2022.
2.	Ray S. Furuya : Does polarization fraction decrease toward shorter wavelength?, BISTRO Consortium Virtual (online) Conference, East Asian Observatory, Nov. 2020.
3.	Ray S. Furuya : The JCMT BISTRO survey: submillimeter polarization spectra of thermal emission from dust grains in high-density star-forming gas, Magnetic Fields in the Universe 7, Quy Nhon, Vietnam, Feb. 2020.
4.	Ray S. Furuya : A first comparison between 850 and 450 micron dust polarization images toward high-density star-forming gas in Ophiuchu A, JCMT Users Meeting 2019, Taipei, Taiwan, R.O.C., Nov. 2019.
5.	Ray S. Furuya : The JCMT BISTRO Survey: A first comparison between 850 and 450 micron dust polarization images toward high-density star-forming gas, Seminário alla Departamento de física e astronomia Universidade do Porto, Porto, Portugal, Oct. 2019.
6.	Ray S. Furuya : Polarization imaging: lessons learned and wishes for future instrumentation, International Workshop on EAO Futures: Future Science and Instrumentation, Nanjing, China, May 2019.
7.	Ray S. Furuya : A comparison of 450 and 850 micron polarization maps towards the center of Ophiuchus A star-forming region, Polarimetry in the ALMA era: a new crossroads of astrophysics, 東京都三鷹市, Mar. 2019.
8.	Ray S. Furuya : Closing remarks, Polarimetry in the ALMA era: a new crossroads of astrophysics, 東京都三鷹市, Mar. 2019.
9.	Ray S. Furuya : Key questions in Interstellar B-field Session, Polarimetry in the ALMA era: a new crossroads of astrophysics, 東京都三鷹市, Mar. 2019.
10.	Ray S. Furuya : Submillimeter dust polarization imaging towards star-forming regions, 国立天文台・理論研究部・理論天文学研究会・収録, Dec. 2018.
11.	Ray S. Furuya : The JCMT BISTRO survey: a first look of 450 micron polarization images, Interstellar filament paradigm: on their formation, evolution, and role in star formation, 名古屋市, Nov. 2018.
12.	Ray S. Furuya : BISTRO(B-fields In STar forming Region Observations) -- A JCMT Large Program with the POL-2 and SCUBA-2 System, Radio Astronomy Group Sminar, Department of Physics, Faculty of Science, The Chinese University of Hong Kong, Mar. 2018.
13.	Ray S. Furuya, Yoshimi Kitamura and Hiroko Shinnaga : A 1000 AU Scale Molecular Outflow Driven by a Candidate First Hydrostatic Core in a filament supported by MHD turbulence, ZENODO, Santiago, Chile, Jun. 2017. (要約) To shed light on the physical properties of a first hydrostatic core, first core, in low-mass protostar formation process, we conducted interferometric observations towards an exceptionally young ''proto"star GF9-2 using the CARMA and SMA. The observations have been carried out in the CO J=3-2 line and in the continuum emission at the wavelengths of 3.3 mm, 1.1 mm and 850 micron with a spatial resolution of ~400 AU. Our spectroscopic imaging of the CO line revealed that the continuum source is driving a 1000 AU scale molecular outflow, including a pair of lobes where a collimated ``higher" velocity (~10 km/s with respect to the velocity of the cloud) red lobe exists inside a poorly collimated ''lower" velocity (~5 km/s) red lobe. These lobes are found to be one of the youngest (dynamical time scales of ~500 - 3000 yrs) and the least powerful (momentum rates of ~10^{-7}-10^{-6} Msun kms/yr) ones so far detected. All the continuum images detected a single point-like source with an effective beam-deconvolve radius of 250 AU at the center of the 3.5 Sun molecular cloud core. Analyzing the spectral energy distribution of the continuum emission, we estimated a ''circum"stellar mass of the gas and dust to be M_csm ~ 8x10^{-3} Msun within ~400 AU in radius, a ''stellar surface" temperature of T* ~ 150 K with an assumption of a ''stellar radius" of 5 AU and a bolometric luminosity of 0.06 Lsun. In addition, a ''stellar" mass of M* < 0.07 +/- 0.02 Msun was estimated using the previously obtained upper limit of the ''stellar" age of tau_* < (2.7 +/- 0.5) x 10^3 yrs and the mass accretion rate of dM/dt_acc = 2.5 x 10^{-5} Msun yr^{-1}. All the observational facts assessed so far reinforces an assertion that the continuum source represents a first core candidate. (出版サイトへのリンク) ● Publication site (DOI): 10.5281/zenodo.808592 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.5281/zenodo.808592 (DOI: 10.5281/zenodo.808592)
14.	Ray S. Furuya and Y. Taniguchi : A Massive Dense Gas Cloud Close to the Nucleus of the Seyfert Galaxy NGC1068, Star Formation from Cores to Clusters, Proceedings of the Conference, Vol.1, 22, Santiago, Chile, Jun. 2017. (要約) Using the ALMA archival data of both CO(6-5) line and 689 GHz continuum emission towards the archetypical Seyfert galaxy, NGC1068, we identified a distinct dense gas separated by 15pc from the AGN, in projection. The continuum flux gives a gas mass of M_gas 2 x 10^5 Msun and bolometric luminosity of 10^8 Lsun, leading to a star formation rate (SFR) of 0.1 M_sun/yr. We found that the gas stands a unique position between galactic and extraglactic clouds in the diagrams of SFR vs. gas mass. All the properties may be understood in terms of the turbulence-regulated star formation scenario. (出版サイトへのリンク) ● Publication site (DOI): 10.5281/zenodo.808590 (文献検索サイトへのリンク) ● Search Scopus @ Elsevier (DOI): 10.5281/zenodo.808590 (DOI: 10.5281/zenodo.808590)
15.	Ray S. Furuya : BISTRO (B-fields In STar forming Region Observations) -- A JCMT Large Program with the POL-2 and SCUBA-2 System, Array Science Center Colloquium, National Radio Astronomical Observatory, Soccorro, NM, U.S.A., Soccorro, NM, U.S.A., Aug. 2016.

国内講演発表:

1.	古屋 S. 玲 : 「銀河中心が駆動する物質エネルギー循環像」を目指して, 銀河系中心研究会2023 (https://sites.google.com/view/gcw2023jp/%E3%83%9B%E3%83%BC%E3%83%A0), 2023年8月.
2.	古屋 S. 玲 : BISTRO Project Status (13), Vol.P105a, 2023年3月.
3.	古屋 S. 玲 : 現在の星形成:最近の観測的研究の進展から, 初代星・初代銀河研究会2022 (https://sites.google.com/view/fsfg2022/), 2022年11月.
4.	古屋 S. 玲 : BISTRO Project Status (12), Vol.P105a, 2022年9月.
5.	古屋 S. 玲 : 大型サブミリ波望遠鏡LST計画・総合議論, 大型サブミリ波望遠鏡LST計画・科学白書全班合同会議, 2022年3月.
6.	古屋 S. 玲 : 大型サブミリ波望遠鏡LST計画・タイムドメイン・サイエンス検討, 大型サブミリ波望遠鏡LST計画・科学白書全班合同会議, 2022年3月.
7.	Ray S. Furuya : Rotating clumps/cores in a magnetically-turbulent filament : a benchmark toward future surveys, ALMA Workshop 2022 -- Synergies between ALMA and wide-field high-cadence multi-wavelength surveys, Mar. 2022.
8.	Ray S. Furuya : Molecular clumps in the magnetically-turbulent OMC-3 filament, 新学術領域「星惑星形成」研究会, Mar. 2022.
9.	古屋 S. 玲 : 東アジア天文台(EAO)の現状と今後の方向性, 2021年度宇宙電波懇談会シンポジウム, 2022年3月.
10.	古屋 S. 玲 : 大型サブミリ波望遠鏡LSTを実現するために ---- 求められる技術, 第22回受信機ワークショップ, 2022年2月.
11.	古屋 S. 玲 : 東アジア天文台(EAO):国際協力のもうひとつの拠点, VLBI懇談会シンポジウム, 2021年11月.
12.	古屋 S. 玲 : 企画セッション「次世代サブミリ波-テラヘルツ地上単一鏡」・総合討論, 日本天文学会秋季年会, 2021年9月.
13.	古屋 S. 玲 : 磁気乱流フィラメントの進化: 分子雲コア形成と星質量を決めるコア重力崩壊の初期条件, 新学術領域「星惑星形成」研究会, 2021年6月.
14.	古屋 S. 玲 : 地上観測天文学者がほしかったもの, ほしいもの, やってきたこと, やりたいこと, 国立天文台データ天文データ解析センター・ユーザーズ・ミーティング, 2021年6月.
15.	古屋 S. 玲 : JCMT SCUBA-2 plus POL-2システムの限界と LSTに求められる直線偏波撮像性能, 国立天文台研究集会「 (サブ)ミリ波単一鏡の革新で挑む, 天文学の未解決問題」, 2021年3月.
16.	長谷川哲夫, 古屋 S. 玲 : BISTRO Project Status (9), 日本天文学会2021年春季年会, No.P126A, 2021年3月.
17.	古屋 S. 玲 : 議論, JCMTワークショップ2021, 2021年1月.
18.	古屋 S. 玲 : 「1日目と2日目の内容紹介」, JCMTワークショップ2021, 2021年1月.
19.	古屋 S. 玲 : 磁気乱流フィラメントの進化: 分子雲コア形成と星質量を決めるコア重力崩壊の初期条件, 新学術領域「星惑星形成」研究会, 2020年10月.
20.	古屋 S. 玲 : What are we learning with the ground-based imaging polarimeter?, Nobeyama Science Workshop 2020, 2020年9月.
21.	古屋 S. 玲 : 地上遠赤外線偏波観測と東アジア天文台:現状と将来, 光学赤外線天文学連絡会シンポジウム2020, 2020年9月.
22.	古屋 S. 玲 : BISTRO:850μm偏波機能付き``SCUBA-3''カメラの製作 (1) 科学目標, 日本天文学会2020年春季年会予稿集, P138a, 2020年3月.
23.	古屋 S. 玲 : BISTRO:星形成領域における450 μm帯ダスト熱放射偏波撮像マップ, 日本天文学会2018年秋季年会予稿集, 2019年9月.
24.	Hasegawa Tetsuo and Ray S. Furuya : BISTRO Project Status (4), 日本天文学会2018年秋季年会予稿集, Sep. 2019.
25.	古屋 S. 玲 : BISTRO:星形成領域における450μm帯ダスト熱放射偏波撮像マップ (2), 日本天文学会2019年秋季年会予稿集, P126a, 2019年9月.
26.	古屋 S. 玲 : サブミリ波単一鏡直線偏波撮像の方法論と誤差評価入門, 偏波の小さな学校, 2019年3月.
27.	Hasegawa Tetsuo, Ray S. Furuya and al. et : BISTRO Project Status (5), 日本天文学会2018年春季年会予稿集, Vol.P110a, Mar. 2019.
28.	古屋 S. 玲 : 「日本学術会議マスタープラン2020 」に向けた宇宙電波コミュニティの意向調査, 2017年度宇宙電波懇談会シンポジウム「未来を拓く技術開発とその将来展望」, 於:国立天文台三鷹, 2018年3月.
29.	古屋 S. 玲 : サブミリ波直線偏波撮像システムSCUBA2+POL2が拓いたdiscovery spaceと次世代装置への課題, 2017年度宇宙電波懇談会シンポジウム「未来を拓く技術開発とその将来展望」, 於:国立天文台三鷹, 2018年3月.
30.	古屋 S. 玲 : 0.01-pc scale View of the Polarization Structure at 850 micron towards Star Forming Regions, 国立天文台研究集会:「星形成と銀河構造における磁場の役割」, 於:鹿児島大学, http://th.nao.ac.jp/MEMBER/kataoka/kagoshima2017/, 2017年12月.
31.	古屋 S. 玲 : BISTRO: A Step towards ALMA Polarization Observations, 於:国立天文台三鷹, 2017年10月.
32.	大西利和, 古屋 S. 玲 : East Asian Observatory, 2016年度宇宙電波懇談会シンポジウム「若手研究者の本音とシニア層の本音:研究の多様性と深さを今後も追求するために」, 於:国立天文台三鷹, 2017年2月.
33.	古屋 S. 玲 : 天文学会キャリア支援委員会を知っていますか?, 2016年度宇宙電波懇談会シンポジウム「若手研究者の本音とシニア層の本音:研究の多様性と深さを今後も追求するために」, 於:国立天文台三鷹, 2017年2月.
34.	古屋 S. 玲 : JCMT搭載サブミリ波偏波計POL-2を用いた星形成領域の網羅的観測(BISTRO)の進捗, 第6回国立天文台理論研究部シンポジウム「星形成を軸に俯瞰する磁場の役割とその観測的検証」, 2016年11月.
35.	古屋 S. 玲 : 趣旨説明, 第6回国立天文台理論研究部シンポジウム「星形成を軸に俯瞰する磁場の役割とその観測的検証」, 2016年11月.
36.	古屋 S. 玲, 齋藤隆仁, 井戸慶治, 宮崎隆義, 饗場和彦, 三好德和, 荒木秀夫, 日野出大輔, 吉本勝彦, 佐々木奈三江 : 徳島大学における「大学入門講座・読書レポート2014」の試み:読書からアカデミック・ライティングへ-, 平成26年度 FD推進プログラム大学教育カンファレンス in 徳島, 2014年12月.
37.	古屋 S. 玲, 齊藤隆仁, 井戸慶治, 宮崎隆義, 饗場和彦, 三好德和, 荒木秀夫, 日野出大輔, 佐々木奈三江 : 徳島大学における「大学入門講座・読書レポート2014」の試み, --- 読書からアカデミック・ライティングへ ---, 平成26年度全学FD 徳島大学教育カンファレンスin徳島, 14-15, 2014年12月. (キーワード) 大学入門講座 / 読書レポート / 新入生 / 附属図書館
38.	古屋 S. 玲, 齊藤隆仁 : 徳島大学における「物理学とその関連分野の教育に関する情報交換会」, --- (通称，物理 FD)の試み ---, 平成26年度全学FD 徳島大学教育カンファレンスin徳島, 14-15, 2014年12月. (キーワード) 物理 / FD
39.	古屋 S. 玲 : 基調講演『徳島大学における「読書レポート」の試み:教科の枠を超えた基礎力とは』, 平成25年度高校と大学の教育内容接続のための情報交換会, 徳島県教育委員会, 於:徳島県立総合教育センター, 2013年12月.

作品:

1.	古屋 S. 玲 : よくばり天文学者たちのよくばりプロジェクト【後編】, アカデミスト・ジャーナル, https://academist-cf.com/journal/?p=1035, 2016年6月.
2.	古屋 S. 玲 : よくばり天文学者たちのよくばりプロジェクト【前編】, アカデミスト・ジャーナル, https://academist-cf.com/journal/?p=1030, 2016年6月.

その他・研究会:

1.	Ray S. Furuya : A first look of 450 micron polarization images with JCMT, Seminari di gruppo Formazione stellare,Osservatorio Astrofisico di Arcetri, Istituto Nazionale di Astrofisica, Sep. 2018.

報告書:

1.	植野美彦, 関陽介, 依岡隆児, 和泉唯信, 二川健, 岡久玲子, 石丸直澄, 尾崎和美, 田中秀治, 寺田賢治, 田中保, 古屋 S. 玲, 上岡麻衣子 : 令和3年度徳島大学高等教育研究センターアドミッション部門報告書, 令和3年度徳島大学高等教育研究センターアドミッション部門報告書, 2022年3月.
2.	植野美彦, 関陽介, 矢部拓也, 米村重信, 阪上浩, 生島仁史, 藤猪英樹, 白山靖彦, 山田健一, 木下和彦, 櫻谷英治, 古屋 S. 玲, 上岡麻衣子 : 令和2年度徳島大学高等教育研究センターアドミッション部門報告書, 令和2年度徳島大学高等教育研究センターアドミッション部門報告書, 2021年3月.
3.	植野美彦, 関陽介, 井戸慶治, 髙木康志, 阪上浩, 生島仁史, 藤猪英樹, 白山靖彦, 田中秀治, 川田昌武, 長宗秀明, 古屋 S. 玲, 上岡麻衣子 : 令和元年度徳島大学高等教育研究センターアドミッション部門報告書, 令和元年度徳島大学高等教育研究センターアドミッション部門報告書, 2020年3月.
4.	植野美彦, 関陽介, 佐藤健二, 野間口雅子, 二川健, 生島仁史, 浜田賢一, 白山靖彦, 山田健一, 古部昭広, 松木均, 古屋 S. 玲, 上岡麻衣子 : 平成30年度徳島大学総合教育センターアドミッション部門報告書, 平成30年度徳島大学総合教育センターアドミッション部門報告書, 徳島, 2019年3月.
5.	植野美彦, 澤田麻衣子, 荒武達朗, 橋本一郎, 二川健, 安井敏之, 浜田賢一, 白山靖彦, 山田健一, 北條昌秀, 音井威重, 古屋 S. 玲, 関陽介 : 平成29年度徳島大学総合教育センターアドミッション部門報告書, 平成29年度徳島大学総合教育センターアドミッション部門報告書, 2018年3月.
6.	植野美彦, 澤田麻衣子, 田島俊郎, 田中克哉, 白山靖彦, 川添和義, 外輪健一郎, 中村嘉利, 古屋 S. 玲 : 平成28年度徳島大学総合教育センターアドミッション部門報告書, 平成28年度徳島大学総合教育センターアドミッション部門報告書, 2017年3月.
7.	Ray S. Furuya and Derek Ward-Thompson : B-fields In STar-forming Region Observations: BISTRO, East Asian Observatory News, No.2, 12-13, Hawaii, Jul. 2016.
8.	佐藤高則, 宮田政徳, 堤和博, 福田利久スティーブ, 齊藤隆仁, 古屋 S. 玲, 吉本勝彦, 三好德和, 荒木秀夫 : 全学共通教育センター FDの歴史, 徳島大学FDの歴史, Vol.2, 91-111, 徳島, 2014年12月.

科学研究費補助金 (KAKEN Grants Database @ NII.ac.jp)

磁気乱流フィラメントの進化：分子雲コア形成と星質量を決めるコア重力崩壊の初期条件 (研究課題/領域番号: 21H00045 )
サブミリ波偏波観測の革新が導く, 磁場を含む星形成ガス像 (研究課題/領域番号: 19H01938 )
なぜ星形成には孤立的と集団的の2つのモードがあるのか? (研究課題/領域番号: 20740113 )
研究者番号（60455201）による検索

准教授 : 古屋玲 S.

研究活動

個人のホームページ

専門分野

研究テーマ

著書・論文

著書:

学術論文(審査論文):

学術論文(紀要・その他):

総説・解説:

国際会議:

国内講演発表:

作品:

その他・研究会:

報告書:

科学研究費補助金 (KAKEN Grants Database @ NII.ac.jp)

准教授 : 古屋 玲 S.

研究活動

個人のホームページ

専門分野

研究テーマ

著書・論文

著書:

学術論文(審査論文):

学術論文(紀要・その他):

総説・解説:

国際会議:

国内講演発表:

作品:

その他・研究会:

報告書:

科学研究費補助金 (KAKEN Grants Database @ NII.ac.jp)

准教授 : 古屋玲 S.