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  1. 理工学研究科
  2. 理工学研究科・学術誌論文

Water Maser Survey on AKARI and IRAS Sources: A Search for "Low-velocity" Water Fountains

http://hdl.handle.net/10232/18718
http://hdl.handle.net/10232/18718
757b655b-2f15-4290-865e-68be881f6fa1
名前 / ファイル ライセンス アクション
IMAI_0004-637X_769_1_20.pdf IMAI_0004-637X_769_1_20.pdf (893.4 kB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2013-07-22
タイトル
タイトル Water Maser Survey on AKARI and IRAS Sources: A Search for "Low-velocity" Water Fountains
著者 Yung, Bosco H. K.

× Yung, Bosco H. K.

WEKO 115751

Yung, Bosco H. K.

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NAKASHIMA, Jun-ichi

× NAKASHIMA, Jun-ichi

WEKO 115752

NAKASHIMA, Jun-ichi

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IMAI, Hiroshi

× IMAI, Hiroshi

WEKO 115753

IMAI, Hiroshi

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DEGUCHI, Shuji

× DEGUCHI, Shuji

WEKO 115754

DEGUCHI, Shuji

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Henkel, Christian

× Henkel, Christian

WEKO 115755

Henkel, Christian

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Kwok, Sun

× Kwok, Sun

WEKO 115756

Kwok, Sun

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著者よみ
姓名 ナカシマ, ジュンイチ
著者よみ
姓名 イマイ, ヒロシ
著者よみ
姓名 デグチ, シュウジ
別言語の著者
姓名 中島, 淳一
別言語の著者
姓名 今井, 裕
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 infrared: stars
キーワード
主題Scheme Other
主題 masers
キーワード
主題Scheme Other
主題 stars: AGB and post-AGB
キーワード
主題Scheme Other
主題 stars: evolution
キーワード
主題Scheme Other
主題 stars: 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 present the results of a 22 GHz H2O maser survey toward a new sample of asymptotic giant branch (AGB) and post-AGB star candidates. Most of the objects are selected for the first time based on the AKARI data, which have high flux sensitivity in the mid-infrared ranges. We aim at finding H2O maser sources in the transient phase between the AGB and post-AGB stages of evolution, where the envelopes start to develop large deviations from spherical symmetry. The observations were carried out with the Effelsberg 100 m radio telescope. Among 204 observed objects, 63 detections (36 new) were obtained. We found four objects that may be "water fountain" sources (IRAS 15193+3132, IRAS 18056–1514, OH 16.3–3.0, and IRAS 18455+0448). They possess an H2O maser velocity coverage much smaller than those in other known water fountains. However, the coverage is still larger than that of the 1612 MHz OH maser. It implies that there is an outflow with a higher velocity than the envelope expansion velocity (typically ≤25 km s^{–1}), meeting the criterion of the water fountain class. We suggest that these candidates are possibly oxygen-rich late AGB or early post-AGB stars in a stage of evolution immediately after the spherically symmetric AGB mass loss has ceased.
収録雑誌名 The Astrophysical Journal

巻 769, 号 1, 発行日 2013
作成日
日付 2013-05-20
ISSN
収録物識別子タイプ ISSN
ISSN 0004-637X
DOI
識別子タイプ DOI
DOI info:doi/10.1088/0004-637X/769/1/20
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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