Study on star formation on spiral arms on the Galaxy through unbiased survey of molecular clouds
Project/Area Number |
18K13580
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Research Category |
Grant-in-Aid for Early-Career Scientists
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Allocation Type | Multi-year Fund |
Review Section |
Basic Section 16010:Astronomy-related
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Research Institution | Osaka Prefecture University (2019-2020) Nagoya University (2018) |
Principal Investigator |
Nishimura Atsushi 大阪府立大学, 理学(系)研究科(研究院), 非常勤研究員 (50738565)
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Project Period (FY) |
2018-04-01 – 2021-03-31
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Project Status |
Completed (Fiscal Year 2020)
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Budget Amount *help |
¥4,030,000 (Direct Cost: ¥3,100,000、Indirect Cost: ¥930,000)
Fiscal Year 2020: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2019: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2018: ¥1,820,000 (Direct Cost: ¥1,400,000、Indirect Cost: ¥420,000)
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Keywords | 星形成 / 大質量星 / 分子雲 / 分子雲衝突 / 電波望遠鏡 / 星間物質 / 電波天文学 |
Outline of Final Research Achievements |
This study aims to understand the origin of star formation efficiency in galaxies. Two observation proposals using Nobeyama 45-m radio telescope were accepted, and distributions of molecular gas in the Galaxy are surveyed.In addition, we developed a method to detect cloud-cloud collision event through detailed investigations of gas kinematics. As a result, a number of candidates where the star formation is triggered by the cloud-cloud collision were found regardless of their location in the galactic structures (e.g., arm or spur). This fact indicates that the star formation efficiency in the Galaxy is probably controlled by the frequency of cloud-cloud collision.
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Academic Significance and Societal Importance of the Research Achievements |
星がどのように生まれるか、は、その後に引き起こされる重元素の生成などを通じて、惑星の起源や生命の誕生に繋がり、宇宙の歴史を紐解く上でも重要な壮大なテーマである。従来、星は、一つの分子雲の中で独立して生まれると素朴に信じられて来た。本研究は、特に大質量星においては、星形成が銀河の中で複数の分子雲が出会い衝突する事を契機に始まる可能性が高い事を観測的に示した。またそれが、銀河内のガス量の大小を問わず、さらには系外銀河においてまで、いかなる場所においても普遍的に同様に起きているであろう事が示された。今後、宇宙における多種多様な星の形成、銀河進化の研究に大きな波及効果を与えると予想される。
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Report
(4 results)
Research Products
(25 results)
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[Journal Article] ALMA Observations of Giant Molecular Clouds in M33. I. Resolving Star Formation Activities in the Giant Molecular Filaments Possibly Formed by a Spiral Shock2020
Author(s)
Tokuda K., Muraoka K., Kondo H., Nishimura A., Tosaki T., Zahorecz S., Onodera S., Miura R. E., Torii K., Kuno N., Fujita S., Sano H., Onishi T., Saigo K., Fukui Y., Kawamura A., Tachihara K.
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Journal Title
The Astrophysical Journal
Volume: 896
Issue: 1
Pages: 36-36
DOI
Related Report
Peer Reviewed / Open Access / Int'l Joint Research
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[Journal Article] FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45 m telescope (FUGIN). VI. Dense gas and mini-starbursts in the W43 giant molecular cloud complex2020
Author(s)
Kohno, Mikito; Tachihara, Kengo; Torii, Kazufumi; Fujita, Shinji; Nishimura, Atsushi; Kuno, Nario; Umemoto, Tomofumi; Minamidani, Tetsuhiro; Matsuo, Mitsuhiro; Kiridoshi, Ryosuke; Tokuda, Kazuki; Hanaoka, Misaki; Tsuda, Yuya; Kuriki, Mika; Ohama, Akio; Sano, Hidetoshi; Hasegawa, Tetsuo; et al.
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Journal Title
Publications of the Astronomical Society of Japan
Volume: 受理済み
Related Report
Peer Reviewed
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[Presentation] ALMA view of 1 pc-scale molecular gas structures in M33 Revealing star-formation activities in molecular filaments/clumps2019
Author(s)
Atsushi NISHIMURA, Kazuyuki MURAOKA, Kazuki TOKUDA, Hiroshi KONDO, Toshikazu ONISHI, Tomoka TOSAKI, Rie MIURA, Kazuki SAIGO, Akiko KAWAMURA, Kazufumi TORII, Sachiko ONODERA, Nario KUNO, Shinji FUJITA, Kengo TACHIHARA, and Yasuo FUKUI
Organizer
ALMA2019: Science Results and Cross-Facility Synergies
Related Report
Int'l Joint Research
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[Presentation] 銀河系 Local Spur における分子ガスの密度進化2019
Author(s)
西村淳, 上田翔汰, 大西利和 (大阪府立大), 藤田真司, 河野樹人, 堤大陸, 立原研悟, 福井康雄 (名古屋 大), 徳田一起 (大阪府立大/国立天文台), 鳥居和史, 宮本祐介, 南谷哲宏, 西合一矢 (国立天文台), 半田 利弘 (鹿児島大)
Organizer
日本天文学会2019年秋季年会
Related Report
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[Presentation] Sagittarius arm における大質量星形成2018
Author(s)
西村淳, 大河一貴, 堤大陸, 河野樹人, 藤田真司, 吉池智史, 大浜晶生, 立原研悟, 福井康雄 (名古屋大 学), 南谷哲宏, 鳥居和史 (国立天文台), 大西利和 (大阪府立大学), 久野成夫 (筑波大学)
Organizer
日本天文学会2018年秋季年会
Related Report
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[Presentation] Cloud collision triggering high-mass star formation in the Sagittarius arm2018
Author(s)
Atsushi Nishimura (Nagoya U), S. Fujita1, M. Kohno1, A. Ohama1, K. Torii2, S. Yoshiike1, D. Tsutsumi1, K. Okawa1, T. Minamidani2, K. Tachihara1, Y. Fukui1 and NANTEN2/FUGIN members (1: Nagoya U, 2: NRO/NAOJ)
Organizer
Workshop: Star Formation Triggered by Cloud-Cloud Collision
Related Report
Int'l Joint Research
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[Presentation] Cloud collision triggering high-mass star formation in the Sagittarius arm2018
Author(s)
Atsushi Nishimura (Nagoya U), S. Fujita1, M. Kohno1, A. Ohama1, K. Torii2, S. Yoshiike1, D. Tsutsumi1, K. Okawa1, T. Minamidani2, K. Tachihara1, Y. Fukui1 and NANTEN2/FUGIN members (1: Nagoya U, 2: NRO/NAOJ)
Organizer
Shells, clouds and star clusters in galaxies
Related Report
Int'l Joint Research
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[Presentation] FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45 m telescope (FUGIN): Filament properties and star formation in M172018
Author(s)
Atsushi Nishimura (Nagoya University), Tetsuhiro Minamidani, Tomofumi Umemoto, Shinji Fujita, Mitsuhiro Matsuo, Yusuke Hattori, Mikito Kohno, Mitsuyoshi Yamagishi, Yuya Tsuda, Mika Kuriki, Nario Kuno, Kazufumi Torii, Daichi Tsutsumi, Kazuki Okawa, Hidetoshi Sano, Kengo Tachihara, Akio Ohama, and Yasuo Fukui
Organizer
Interstellar filament paradigm: On their formation, evolution, and role in star formation
Related Report
Int'l Joint Research
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