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  1. 100 全学教育機構 (School of General Education)
  2. 1001 学術論文 (Journal Articles)

SPECTROSCOPY ALONG MULTIPLE, LENSED SIGHT LINES THROUGH OUTFLOWING WINDS IN THE QUASAR SDSS J1029+2623

http://hdl.handle.net/10091/17262
792b8375-f3c4-46d9-81b2-9526e4ae9166
プレビュー
名前 / ファイル ライセンス Actions
2013_AJ_145_48.pdf 2013_AJ_145_48.pdf (1.0 MB)
item type 学術雑誌論文 / Journal Article(1)
公開日 2013-12-02
タイトル
タイトル SPECTROSCOPY ALONG MULTIPLE, LENSED SIGHT LINES THROUGH OUTFLOWING WINDS IN THE QUASAR SDSS J1029+2623
言語
言語 eng
キーワード
主題 quasars: absorption lines
キーワード
主題 quasars: individual (SDSS J1029+2623)
資源タイプ
資源 http://purl.org/coar/resource_type/c_6501
タイプ journal article
著者 Misawa, Toru

× Misawa, Toru

WEKO 45860

Misawa, Toru

Search repository
Inada, Naohisa

× Inada, Naohisa

WEKO 45861

Inada, Naohisa

Search repository
Ohsuga, Ken

× Ohsuga, Ken

WEKO 45862

Ohsuga, Ken

Search repository
Gandhi, Poshak

× Gandhi, Poshak

WEKO 45863

Gandhi, Poshak

Search repository
Takahashi, Rohta

× Takahashi, Rohta

WEKO 45864

Takahashi, Rohta

Search repository
Oguri, Masamune

× Oguri, Masamune

WEKO 45865

Oguri, Masamune

Search repository
信州大学研究者総覧へのリンク
Misawa, Toru
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 ASTRONOMICAL JOURNAL. 145(2):48 (2013)
書誌情報 ASTRONOMICAL JOURNAL

巻 145, 号 2, p. 48, 発行日 2013-02
抄録
内容記述タイプ Abstract
内容記述 We study the origin of absorption features on the blue side of the C IV broad emission line of the large-separation lensed quasar SDSS J1029+2623 at z(em) similar to 2.197. The quasar images, produced by a foreground cluster of galaxies, have a maximum separation angle of theta similar to 22 ''.5. The large angular separation suggests that the sight lines to the quasar central source can go through different regions of outflowing winds from the accretion disk of the quasar, providing a unique opportunity to study the structure of outflows from the accretion disk, a key ingredient for the evolution of quasars as well as for galaxy formation and evolution. Based on medium- and high-resolution spectroscopy of the two brightest images conducted at the Subaru telescope, we find that each image has different intrinsic levels of absorptions, which can be attributed either to variability of absorption features over the time delay between the lensed images, Delta t similar to 744 days, or to the fine structure of quasar outflows probed by the multiple sight lines toward the quasar. While both these scenarios are consistent with the current data, we argue that they can be distinguished with additional spectroscopic monitoring observations.
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 0004-6256
書誌レコードID
収録物識別子タイプ NCID
収録物識別子 AA00552749
DOI
関連識別子
識別子タイプ DOI
関連識別子 http://dx.doi.org/10.1088/0004-6256/145/2/48
関連名称
関連名称 10.1088/0004-6256/145/2/48
権利
権利情報 Copyright© 2013 The American Astronomical Society
著者版フラグ
値 publisher
WoS
Web of Science
http://gateway.isiknowledge.com/gateway/Gateway.cgi?&GWVersion=2&SrcAuth=ShinshuUniv&SrcApp=ShinshuUniv&DestLinkType=FullRecord&DestApp=WOS&KeyUT=000313571600022
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