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ヒラノ シンゴ
Hirano Shingo 平野 信吾 所属 神奈川大学 工学部 応用物理学科 職種 助教 |
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| 言語種別 | 英語 |
| 発行・発表の年月 | 2023/11 |
| 形態種別 | 学術雑誌 |
| 査読 | 査読あり |
| 標題 | Secondary Outflow Driven by the Protostar Ser-emb 15 in Serpens |
| 執筆形態 | 共著 |
| 掲載誌名 | The Astrophysical Journal |
| 掲載区分 | 国外 |
| 出版社・発行元 | American Astronomical Society |
| 巻・号・頁 | 958(2),pp.102-119 |
| 国際共著 | 国際共著 |
| 著者・共著者 | ◎Asako Sato,Kazuki Tokuda,Masahiro N. Machida,Kengo Tachihara,Naoto Harada,Hayao Yamasaki,Shingo Hirano,Toshikazu Onishi,Yuko Matsushita |
| 概要 | Abstract
We present the detection of a secondary outflow associated with a Class I source, Ser-emb 15, in the Serpens Molecular Cloud. We reveal two pairs of molecular outflows consisting of three lobes, that is, primary and secondary outflows, using Atacama Large Millimeter/submillimeter Array 12CO and SiO line observations at a resolution of ~318 au. The secondary outflow is elongated approximately perpendicular to the axis of the primary outflow in the plane of the sky. We also identify two compact structures, Sources A and B, within an extended structure associated with Ser-emb 15 in the 1.3 mm continuum emission at a resolution of ∼40 au. The projected sizes of Sources A and B are 137 au and 60 au, respectively. Assuming a dust temperature of 20 K, we estimate the dust mass to be 2.4e-3 Msun for Source A and 3.3e-4 Msun for Source B. |
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