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  1. B100 理学部/理学研究科
  2. B100a 雑誌掲載論文
  3. 学術雑誌

Evidence for a cloud–cloud collision in Sh2-233 triggering the formation of the high-mass protostar object IRAS 05358+3543

http://hdl.handle.net/2237/0002004248
http://hdl.handle.net/2237/0002004248
046654a6-cae2-4585-b008-ee51d1b27a6b
名前 / ファイル ライセンス アクション
stac1087.pdf stac1087.pdf (4.1 MB)
Item type itemtype_ver1(1)
公開日 2022-12-01
タイトル
タイトル Evidence for a cloud–cloud collision in Sh2-233 triggering the formation of the high-mass protostar object IRAS 05358+3543
言語 en
著者 Yamada, Rin I

× Yamada, Rin I

en Yamada, Rin I

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Fukui, Yasuo

× Fukui, Yasuo

en Fukui, Yasuo

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Sano, Hidetoshi

× Sano, Hidetoshi

en Sano, Hidetoshi

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Tachihara, Kengo

× Tachihara, Kengo

en Tachihara, Kengo

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Bieging, John H

× Bieging, John H

en Bieging, John H

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Enokiya, Rei

× Enokiya, Rei

en Enokiya, Rei

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Nishimura, Atsushi

× Nishimura, Atsushi

en Nishimura, Atsushi

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Fujita, Shinij

× Fujita, Shinij

en Fujita, Shinij

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Kohno, Mikito

× Kohno, Mikito

en Kohno, Mikito

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Tsuge, Kisetsu

× Tsuge, Kisetsu

en Tsuge, Kisetsu

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アクセス権
アクセス権 open access
アクセス権URI http://purl.org/coar/access_right/c_abf2
権利
言語 en
権利情報 This article has been accepted for publication in [Monthly Notices of the Royal Astronomical Society] ©: [2022] [authors] Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
キーワード
主題Scheme Other
主題 stars: formation
キーワード
主題Scheme Other
主題 ISM: clouds
キーワード
主題Scheme Other
主題 ISM: individual objects: IRAS 05358+3543
内容記述
内容記述 We have carried out a new kinematical analysis of the molecular gas in the Sh2-233 region by using the CO J = 2–1 data taken at ∼0.5 pc resolution. The molecular gas consists of a filamentary cloud of 5-pc length with 1.5-pc width where two dense cloud cores are embedded. The filament lies between two clouds, which have a velocity difference of 2.7 km s−1 and are extended over ∼5 pc. We frame a scenario that the two clouds are colliding with each other and compressed the gas between them to form the filament in ∼0.5 Myr which is perpendicular to the collision. It is likely that the collision formed not only the filamentary cloud but also the two dense cores. One of the dense cores is associated with the high-mass protostellar candidate IRAS 05358+3543, a representative high-mass protostar. In the monolithic collapse scheme of high mass star formation, a compact dense core of 100 M⊙ within a volume of 0.1 pc radius is assumed as the initial condition, whereas the formation of such a core remained unexplained in the previous works. We argue that the proposed collision is a step which efficiently collects the gas of 100 M⊙ into 0.1 pc radius. This lends support for that the cloud–cloud collision is an essential process in forming the compact high-mass dense core, IRAS 05358+3543.
言語 en
内容記述タイプ Abstract
出版者
言語 en
出版者 Oxford University Press
言語
言語 eng
資源タイプ
資源タイプresource http://purl.org/coar/resource_type/c_6501
タイプ journal article
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
関連情報
関連タイプ isVersionOf
識別子タイプ DOI
関連識別子 https://doi.org/10.1093/mnras/stac1087
収録物識別子
収録物識別子タイプ PISSN
収録物識別子 0035-8711
書誌情報 en : Monthly Notices of the Royal Astronomical Society

巻 515, 号 1, p. 1012-1025, 発行日 2022-09
ファイル公開日
日付 2022-12-01
日付タイプ Available
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