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  1. 理工学研究科
  2. 理工学研究科・学術誌論文

LINEAR POLARIZATION OBSERVATIONS OF WATER MASERS IN W3 IRS 5

http://hdl.handle.net/10232/26178
http://hdl.handle.net/10232/26178
093d7226-6241-4dd7-8d6f-222854ca6b28
名前 / ファイル ライセンス アクション
Linear Linear Polarization Observations of Water Masers in W3 IRS 5.pdf (708.4 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 LINEAR POLARIZATION OBSERVATIONS OF WATER MASERS IN W3 IRS 5
著者 IMAI, Hiroshi

× IMAI, Hiroshi

WEKO 115976

IMAI, Hiroshi

Search repository
HORIUCHI, Shinji

× HORIUCHI, Shinji

WEKO 115977

HORIUCHI, Shinji

Search repository
DEGUCHI, Shinji

× DEGUCHI, Shinji

WEKO 115978

DEGUCHI, Shinji

Search repository
KAMEYA, Osamu

× KAMEYA, Osamu

WEKO 115979

KAMEYA, Osamu

Search repository
別言語の著者
姓名 今井, 裕
別言語の著者
姓名 堀内, 真司
別言語の著者
姓名 出口, 修至
別言語の著者
姓名 亀谷, 收
言語
言語 eng
キーワード
主題Scheme Other
主題 ISM
キーワード
主題Scheme Other
主題 individual (W3 IRS 5) -- ISM
キーワード
主題Scheme Other
主題 jets and outflows -- masers -- stars
キーワード
主題Scheme Other
主題 formation
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 present a magnetic field mapping of water maser clouds in the star-forming region W3 IRS 5, which has been made on the basis of the linear polarization VLBI observation. Using the Very Long Baseline Array at 22.2 GHz, 16 of 61 detected water masers were found to be linearly polarized with polarization degrees up to 13%. Although 10 polarized features were widely distributed in the whole W3 IRS 5 water maser region, they had position angles similar to the magnetic field vectors (~75° east from the north). The magnetic field vectors are roughly perpendicular to the spatial alignments of the maser features. They are consistent with the hourglass model of the magnetic field, which was previously proposed to explain the magnetic field in the whole W3 Main region (r ~ 0.1 pc). They are, on the other hand, not aligned to the directions of maser feature proper motions observed previously. This implies that the W3 IRS 5 magnetic field was controlled by a collapse of theW3 Main molecular cloud rather than by the outflow originated from W3 IRS 5.
収録雑誌名 The Astronomical Journal

巻 595, 号 1, p. 285-293, 発行日 2003
作成日
日付 2003-09-20
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/10.1086/377198
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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