言語種別 | 英語 |
発行・発表の年月 | 2022/02 |
形態種別 | 学術雑誌 |
査読 | 査読あり |
標題 | Star burst in W49N presumably induced by cloud–cloud collision
Star burst in W49N presumably induced by cloud–cloud collision
|
執筆形態 | 共著 |
掲載誌名 | Publications of the Astronomical Society of Japan |
掲載区分 | 国外 |
出版社・発行元 | The Astronomical Society of Japan |
巻・号・頁 | 74(1),pp.128-151 |
担当範囲 | 解析,論文作成 |
著者・共著者 | Ryosuke Miyawaki, Masahiko Hayashi, Tetsuo Hasegawa
Ryosuke Miyawaki, Masahiko Hayashi, Tetsuo Hasegawa
|
概要 | We present high-resolution observations of CS (J = 1–0), H13CO+ (J = 1–0), and SiO (v = 0: J = 1–0) lines, together with the 49 GHz and 86 GHz continuum emissions, toward W 49 N carried out with the Nobeyama Millimeter Array. We propose a view that two pre-existing clouds with radial velocities of 4 km s−1 and 12 km s−1 collided with each other almost face-on to produce the observed clumps with intermediate velocities and triggered the burst of massive star formation in W 49 N. |
DOI | https://doi.org/10.1093/pasj/psab113 |
researchmap用URL | https://academic.oup.com/pasj/advance-article/doi/10.1093/pasj/psab113/6449105 |