Effect of environment in star formation investigated with adaptive mesh refinement
Project/Area Number |
26400233
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Research Category |
Grant-in-Aid for Scientific Research (C)
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Allocation Type | Multi-year Fund |
Section | 一般 |
Research Field |
Astronomy
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Research Institution | Hosei University |
Principal Investigator |
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Co-Investigator(Renkei-kenkyūsha) |
INUTSUKA Shu-ichiro 名古屋大学, 大学院理学研究科, 教授 (80270453)
MACHIDA Masahiro 九州大学, 大学院理学研究科, 准教授 (10402786)
DOBASHI Kazuhito 東京学芸大学, 教育学部, 教授 (20237176)
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Project Period (FY) |
2014-04-01 – 2017-03-31
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Project Status |
Completed (Fiscal Year 2016)
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Budget Amount *help |
¥4,420,000 (Direct Cost: ¥3,400,000、Indirect Cost: ¥1,020,000)
Fiscal Year 2016: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2015: ¥1,430,000 (Direct Cost: ¥1,100,000、Indirect Cost: ¥330,000)
Fiscal Year 2014: ¥1,820,000 (Direct Cost: ¥1,400,000、Indirect Cost: ¥420,000)
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Keywords | 星形成 / 分子雲 / 分子雲コア / 原始連星 / 原始星 / MHD / 数値シミュレーション / AMR / 星周円盤 / ALMA望遠鏡 |
Outline of Final Research Achievements |
We have studied star formation in the several environments, i.e., different levels of turbulence and magnetic fields. We have performed large-scale numerical simulations with adaptive mesh refinement (AMR), which allows us to obtain a local high resolution. Several models were investigated: cloud interaction (cloud-cloud collision), protostar formation starting from a cloud scale, and circumbinary structure. The results of the numerical simulations were compared with the recent high-resolution observation with ALMA and the 45 m telescope at Nobeyama Radio Observatory. By comparison between the numerical simulations and the observation, we discussed several phenomena in the molecular cloud Cyg OB 7, the high-density molecular cloud core MC27, and protobinary stars L1551 NE.
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Report
(4 results)
Research Products
(26 results)
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[Journal Article] Spiral Arms, Infall, and Misalignment of the Circumbinary Disk from the Circumstellar Disks in the Protostellar Binary System L1551 NE2016
Author(s)
Takakuwa, Shigehisa; Saigo, Kazuya; Matsumoto, Tomoaki; Saito, Masao; Lim, Jeremy; Hanawa, Tomoyuki; Yen, Hsi-Wei; Ho, Paul T. P.
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Journal Title
The Astrophysical Journal
Volume: 837
Issue: 1
Pages: 86-99
DOI
Related Report
Peer Reviewed / Open Access / Int'l Joint Research
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[Journal Article] Revealing a Detailed Mass Distribution of a High-density Core MC27/L1521F in Taurus with ALMA2016
Author(s)
Tokuda, K., Onishi, T., Matsumoto, T., Saigo, K., Kawamura, A., Fukui, Y., Inutsuka, S.-i., Machida, M. N., Tomida, K., Tachihara, K., and Andre, P.
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Journal Title
The Astrophysical Journal
Volume: 826
Issue: 1
Pages: 26-35
DOI
Related Report
Peer Reviewed / Open Access / Int'l Joint Research / Acknowledgement Compliant
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[Journal Article] ALMA Observations of a High-density Core in Taurus : Dynamical Gas Interaction at the Possible Site of a Multiple Star Formation2014
Author(s)
K. Tokuda, T. Onishi, K. Saigo, A. Kawamura, Y. Fukui, T. Matsumoto, S.-i. Inutsuka, M, N. Machida, K. Tomida, K. Tachihara
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Journal Title
The Astrophysical Journal Letters
Volume: 789
Issue: 1
Pages: L4-L4
DOI
Related Report
Peer Reviewed
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