言語種別 | 英語 |
発行・発表の年月 | 2019/02 |
形態種別 | 学術雑誌 |
査読 | 査読あり |
標題 | Molecular Cloud Cores in the Galactic Center 50 km s‑1 Molecular Cloud
Molecular Cloud Cores in the Galactic Center 50 km s‑1 Molecular Cloud
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執筆形態 | 共著 |
掲載誌名 | Astrophysical Journal |
掲載区分 | 国外 |
出版社・発行元 | The American Astronomical Society |
巻・号・頁 | 872(2),pp.121-146 |
担当範囲 | Data Reduction, Discussion |
著者・共著者 | Uehara, Kenta; Tsuboi, Masato; Kitamura, Yoshimi; Miyawaki, Ryosuke; Miyazaki, Atsushi
Uehara, Kenta; Tsuboi, Masato; Kitamura, Yoshimi; Miyawaki, Ryosuke; Miyazaki, Atsushi
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概要 | We observed the whole of the 50MC with a high angular resolution (∼2.″0 × 1.″4) in Atacama Large Millimeter/submillimeter Array cycle 1 in the H13CO+ J = 1‑0 and C34S J = 2‑1 emission lines. We identified 241 and 129 bound cores with a virial parameter of less than 2, which are thought to be gravitationally bound, in the H13CO+ and C34S maps using the clumpfind algorithm, respectively. In the CCC region, the bound H13CO+ and C34S cores are 119 and 82, whose masses are 68% and 76% of those in the whole 50MC, respectively. The distribution of the core number and column densities in the CCC are biased to larger densities than those in the non-CCC region. The distributions indicate that the CCC compresses the molecular gas and increases the number of the dense bound cores. |
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