| 言語種別 | 日本語 |
| 発行・発表の年月 | 2021/08 |
| 形態種別 | 学術雑誌 |
| 査読 | 査読あり |
| 標題 | Hot molecular core candidates in the Galactic center 50 km s-1 molecular cloud
|
| 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 | 73,943-969頁 |
| 著者・共著者 | Ryosuke Miyawaki, Masato Tsuboi, Kenta Uehara, Atsushi Miyazaki
|
| 概要 | We present results based on 2′′.5-resolution observations using the Atacama Large Millimeter/Submillmeter Array (ALMA) of the Galactic center molecular cloud G−0.02−0.07, or the 50 km s−1 molecular cloud (50 MC), in the SO (NJ = 22–11) line and 86 GHz continuum emission, the combination of which is considered to trace “hot molecular core candidates” (HMCCs) appearing in the early stage of massive-star formation. In |
| researchmap用URL | https://academic.oup.com/pasj/advance-article/doi/10.1093/pasj/psab056/6307941 |