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  1. 100 教育・学生支援機構, 全学教育センター
  2. 1001 学術論文

RESOLVING THE CLUMPY STRUCTURE OF THE OUTFLOW WINDS IN THE GRAVITATIONALLY LENSED QUASAR SDSS J1029+2623

http://hdl.handle.net/10091/18076
http://hdl.handle.net/10091/18076
3ae86751-55c4-4c4b-b3ae-fea3de441ce0
名前 / ファイル ライセンス アクション
RESOLVING_THE_CLUMPY_STRUCTURE.pdf RESOLVING_THE_CLUMPY_STRUCTURE.pdf (516.3 kB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2015-02-09
タイトル
タイトル RESOLVING THE CLUMPY STRUCTURE OF THE OUTFLOW WINDS IN THE GRAVITATIONALLY LENSED QUASAR SDSS J1029+2623
言語
言語 eng
DOI
関連識別子 https://doi.org/10.1088/2041-8205/794/2/L20
関連名称 10.1088/2041-8205/794/2/L20
キーワード
主題 quasars: absorption lines, 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

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Misawa, Toru

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Inada, Naohisa

× Inada, Naohisa

Inada, Naohisa

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Oguri, Masamune

× Oguri, Masamune

Oguri, Masamune

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Gandhi, Poshak

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Gandhi, Poshak

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Horiuchi, Takashi

× Horiuchi, Takashi

Horiuchi, Takashi

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Koyamada, Suzuka

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Koyamada, Suzuka

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Okamoto, Rina

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Okamoto, Rina

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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 Astrophys. J. Lett. 794(2):L20 (2014)
書誌情報 ASTROPHYSICAL JOURNAL LETTERS

巻 794, 号 2, p. L20, 発行日 2014-10-20
抄録
内容記述 We study the geometry and the internal structure of the outflowing wind from the accretion disk of a quasar by observing multiple sightlines with the aid of strong gravitational lensing. Using Subaru/High Dispersion Spectrograph, we performed high-resolution (R ~ 36,000) spectroscopic observations of images A and B of the gravitationally lensed quasar SDSS J1029+2623 (at z em ~ 2.197) whose image separation angle, θ ~ 22.''5, is the largest among those discovered so far. We confirm that the difference in absorption profiles in images A and B discovered by Misawa et al. has remained unchanged since 2010, implying the difference is not due to time variability of the absorption profiles over the delay between the images, Δt ~ 744 days, but rather due to differences along the sightlines. We also discovered a time variation of C IV absorption strength in both images A and B due to a change in the ionization condition. If a typical absorber's size is smaller than its distance from the flux source by more than five orders of magnitude, it should be possible to detect sightline variations among images of other smaller separation, galaxy-scale gravitationally lensed quasars.
資源タイプ(コンテンツの種類)
ISSN
収録物識別子タイプ ISSN
収録物識別子 2041-8205
書誌レコードID
収録物識別子タイプ NCID
収録物識別子 AA00553264
権利
権利情報 © 2014. 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
URL http://gateway.isiknowledge.com/gateway/Gateway.cgi?&GWVersion=2&SrcAuth=ShinshuUniv&SrcApp=ShinshuUniv&DestLinkType=FullRecord&DestApp=WOS&KeyUT=000343399200002
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Cite as

Misawa, Toru, Inada, Naohisa, Oguri, Masamune, Gandhi, Poshak, Horiuchi, Takashi, Koyamada, Suzuka, Okamoto, Rina, 2014, RESOLVING THE CLUMPY STRUCTURE OF THE OUTFLOW WINDS IN THE GRAVITATIONALLY LENSED QUASAR SDSS J1029+2623: IOP PUBLISHING LTD, L20– p.

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