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  1. 100 全学教育センター
  2. 1001 学術論文

THE WIDE-ANGLE OUTFLOW OF THE LENSED z=1.51 AGN HS 0810+2554

http://hdl.handle.net/10091/00021879
http://hdl.handle.net/10091/00021879
61142be2-3d2a-4bbc-8eb4-a2b6889e1fb7
名前 / ファイル ライセンス アクション
15K05020_04.pdf 15K05020_04.pdf (1.4 MB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2020-02-28
タイトル
言語 en
タイトル THE WIDE-ANGLE OUTFLOW OF THE LENSED z=1.51 AGN HS 0810+2554
言語
言語 eng
キーワード
主題Scheme Other
主題 galaxies: evolution
キーワード
主題Scheme Other
主題 galaxies: formation
キーワード
主題Scheme Other
主題 intergalactic medium
キーワード
主題Scheme Other
主題 quasars: absorption lines
キーワード
主題Scheme Other
主題 X-rays: galaxies
資源タイプ
資源 http://purl.org/coar/resource_type/c_6501
タイプ journal article
著者 Chartas, G.

× Chartas, G.

WEKO 109024

Chartas, G.

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Cappi, M.

× Cappi, M.

WEKO 109025

Cappi, M.

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Hamann, F.

× Hamann, F.

WEKO 109026

Hamann, F.

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Eracleous, M.

× Eracleous, M.

WEKO 109027

Eracleous, M.

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Strickland, S.

× Strickland, S.

WEKO 109028

Strickland, S.

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Giustini, M.

× Giustini, M.

WEKO 109029

Giustini, M.

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Misawa, T.

× Misawa, T.

WEKO 109030

Misawa, T.

Search repository
信州大学研究者総覧へのリンク
氏名 Misawa, Toru
URL http://soar-rd.shinshu-u.ac.jp/profile/ja.ypchuUkV.html
出版者
出版者 IOP PUBLISHING LTD
引用
内容記述タイプ Other
内容記述 ASTROPHYSICAL JOURNAL.824(1):53(2016)
書誌情報 ASTROPHYSICAL JOURNAL

巻 824, 号 1, p. 53, 発行日 2016-06-10
抄録
内容記述タイプ Abstract
内容記述 We present results from X-ray observations of the gravitationally lensed z - 1.51 active galactic nucleus (AGN) HS 0810+2554 performed with the Chandra X-ray Observatory and XMM-Newton. Blueshifted absorption lines are detected in both observations at rest-frame energies ranging between similar to 1 and 12 keV at greater than or similar to 99% confidence. The inferred velocities of the outflowing components range between similar to 0.1c and similar to 0.4c. A strong emission line at similar to 6.8 keV that is accompanied by a significant absorption line at similar to 7.8 keV is also detected in the Chandra observation. The presence of these lines is a characteristic feature of a P-Cygni profile supporting the presence of an expanding, outflowing, highly ionized iron absorber in this quasar. Modeling of the P-Cygni profile constrains the covering factor of the wind to be greater than or similar to 0.6, assuming disk shielding. A disk-reflection component is detected in the XMM-Newton observation accompanied by blueshifted absorption lines. The XMM-Newton observation constrains the inclination angle to be <45 degrees at 90% confidence, assuming that the hard excess is due to blurred reflection from the accretion disk. The detection of an ultrafast and wide-angle wind in an AGN with intrinsic narrow absorption lines (NALs) would suggest that quasar winds may couple efficiently with the intergalactic medium and provide significant feedback if ubiquitous in all NAL and broad absorption line (BAL) quasars. We estimate the mass-outflow rate of the absorbers to lie in the range of 1.5-3.4M(circle dot) yr(-1) for the two observations. We find that the fraction of kinetic to electromagnetic luminosity released by HS 0810+2554 is large (epsilon(k) = 9(-6)(+8)), which suggests that magnetic driving is likely a significant contributor to the acceleration of this outflow.
資源タイプ(コンテンツの種類)
内容記述タイプ Other
内容記述 Article
ISSN
収録物識別子タイプ ISSN
収録物識別子 0004-637X
書誌レコードID
収録物識別子タイプ NCID
収録物識別子 AA00553242
DOI
識別子タイプ DOI
関連識別子 https://doi.org/10.3847/0004-637X/824/1/53
関連名称 10.3847/0004-637X/824/1/53
権利
権利情報 © 2016. The American Astronomical Society. All rights reserved.
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
WoS
表示名 Web of Science
URL http://gateway.isiknowledge.com/gateway/Gateway.cgi?&GWVersion=2&SrcAuth=ShinshuUniv&SrcApp=ShinshuUniv&DestLinkType=FullRecord&DestApp=WOS&KeyUT=000377937300053
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