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  1. 理工学研究科
  2. 理工学研究科・学術誌論文

A BICONICALLY EXPANDING FLOW IN W43A TRACED BY SiO MASER EMISSION

http://hdl.handle.net/10232/26179
http://hdl.handle.net/10232/26179
ba92e9cc-b0f9-4cf9-be5a-b366b8b0ab00
名前 / ファイル ライセンス アクション
A A Biconically Expanding Flow in W43A Traced by SiO Maser Emission.pdf (341.9 kB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2016-03-15
タイトル
タイトル A BICONICALLY EXPANDING FLOW IN W43A TRACED BY SiO MASER EMISSION
著者 IMAI, Hiroshi

× IMAI, Hiroshi

WEKO 115019

IMAI, Hiroshi

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NAKASHIMA, Jun-ichi

× NAKASHIMA, Jun-ichi

WEKO 115020

NAKASHIMA, Jun-ichi

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DIAMOND, Philip J.

× DIAMOND, Philip J.

WEKO 115021

DIAMOND, Philip J.

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MIYAZAKI, Atsushi

× MIYAZAKI, Atsushi

WEKO 115022

MIYAZAKI, Atsushi

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DEGUCHI, Shuji

× DEGUCHI, Shuji

WEKO 115023

DEGUCHI, Shuji

Search repository
別言語の著者
姓名 今井, 裕
別言語の著者
姓名 中島, 淳一
別言語の著者
姓名 宮崎, 敦史
別言語の著者
姓名 出口, 修至
言語
言語 eng
キーワード
主題Scheme Other
主題 masers -- stars
キーワード
主題Scheme Other
主題 mass loss -- stars
キーワード
主題Scheme Other
主題 individual (W43A) -- stars
キーワード
主題Scheme Other
主題 winds, outflows
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_6501
資源タイプ journal article
要約(Abstract)
内容記述タイプ Other
内容記述 We report Very Long Baseline Array and Very Large Array observations of 22 GHz H2O and 43 GHz SiO (v = 1, J = 1-0) maser emission as well as 7 mm continuum emission in W43A, which exhibits a highly collimated jet of molecular gas and a spherically expanding envelope very similar to that of an OH/IR star. The spatiokinematical structure of the H2O masers is well fitted to a precessing jet model with an expansion velocity of 150 km s^-1 and a dynamical age of ~50 yr. The spatiokinematical structure of the SiO masers is well fitted to a biconically expanding flow model, whose axis is parallel to the direction of the collimated jet. Astrometry of the H2O and SiO masers suggests that these maser sources have a common dynamical center, possibly as part of a binary system, within 70 AU. The SiO masers may be excited on the surface of the cone that has significant deceleration and interacts with the jet. A 7 mm continuum emission source is located ∼1300 AU away from these maser sources at a position angle of about -60° from the jet axis. The physical relation of the continuum to the maser sources is still unclear.
収録雑誌名 The Astronomical Journal

巻 622, 号 2, p. L125-L128, 発行日 2005
作成日
日付 2005-04-01
ISSN
収録物識別子タイプ ISSN
ISSN 0004-6256
NII書誌ID(雑誌)
収録物識別子タイプ NCID
NC ID AA00552749
DOI
識別子タイプ DOI
DOI info:doi/10.1086/429820
権利
権利情報 American Astronomical Society
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
NDC
主題Scheme NDC
主題 440
公開者・出版者
出版者 American Astronomical Society
公開者・出版者
出版者 IOP Publishing
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