言語種別 | 英語 |
発行・発表の年月 | 2023/02 |
形態種別 | 学術雑誌 |
査読 | 査読あり |
標題 | An expanding ring of the hypercompact H ii region W 49 N:A2
An expanding ring of the hypercompact H ii region W 49 N:A2
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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 | Oxford University Press |
巻・号・頁 | 75(1),pp.225-232 |
総ページ数 | 13 |
担当範囲 | 執筆,データ解析 |
担当区分 | 筆頭著者,責任著者 |
著者・共著者 | ◎Ryosuke Miyawaki, Masahiko Hayashi, Tetsuo Hasegawa
◎Ryosuke Miyawaki, Masahiko Hayashi, Tetsuo Hasegawa
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概要 | We present 250 GHz continuum and H29α line data toward W 49 N:A2, a hypercompact H ii region ionized by an O9 star. The data obtained with ALMA at a resolution of ∼0".05 (600 au) confirmed the presence of an ionized ring with a radius of ∼700 au. It has a width of ∼1000 au and is relatively flat with a scale height of less than several hundred au with a velocity of 13.2 km/s. The ring also shows a hint of rotation at 2.7 km/s, which is significantly (2.5 σ) smaller than the Kepler velocity of 5.2 km/s at its radius around the 20 M⊙ star. This can be interpreted as that the ring gas has been transported from the radius of ∼170 au by conserving its original specific angular momentum that it had there. The ionized ring may thus be a remnant of the accretion disk that fed the O9 star. The data has revealed a rare example of how a massive star terminates its accretion at the end of its formation, transforming a hypercompact H ii region into an ultracompact H ii region. |
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