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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 | 2023/03 |
| 形態種別 | 学術雑誌 |
| 査読 | 査読あり |
| 標題 | Crescent-shaped Molecular Outflow from the Intermediate-mass Protostar DK Cha Revealed by ALMA |
| 執筆形態 | 共著 |
| 掲載誌名 | The Astrophysical Journal |
| 出版社・発行元 | American Astronomical Society |
| 巻・号・頁 | 945(1),pp.63-63 |
| 著者・共著者 | ◎Naoto Harada,Kazuki Tokuda,Hayao Yamasaki,Asako Sato,Mitsuki Omura,Shingo Hirano,Toshikazu Onishi,Kengo Tachihara,Masahiro N. Machida |
| 概要 | Abstract
We report on an Atacama Large Millimeter/submillimeter Array study of the Class I or II intermediate-mass protostar DK Cha in the Chamaeleon II region. The 12CO(J = 2-1) images have an angular resolution of ~1 (~250 au) and show high-velocity blueshifted (>=70 km s-1) and redshifted (>=50 km s-1) emissions, which have 3000 au scale crescent-shaped structures around the protostellar disk traced in the 1.3 mm continuum. Because the high-velocity components of the CO emission are associated with the protostar, we concluded that the emission traces the pole-on outflow. |
| DOI | 10.3847/1538-4357/acb930 |
| ISSN | 0004-637X/1538-4357 |
| PermalinkURL | https://iopscience.iop.org/article/10.3847/1538-4357/acb930 |
| researchmap用URL | https://iopscience.iop.org/article/10.3847/1538-4357/acb930/pdf |
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