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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

Spectroscopic Observations of the Outflowing Wind in the Lensed Quasar SDSS J1001+5027

http://hdl.handle.net/10091/00021877
http://hdl.handle.net/10091/00021877
a957694c-172e-4817-a146-44d097b6edf0
名前 / ファイル ライセンス アクション
15K05020_01.pdf 15K05020_01.pdf (1.1 MB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2020-02-28
タイトル
タイトル Spectroscopic Observations of the Outflowing Wind in the Lensed Quasar SDSS J1001+5027
言語
言語 eng
DOI
関連識別子 https://doi.org/10.3847/1538-4357/aaa66e
関連名称 10.3847/1538-4357/aaa66e
キーワード
主題 quasars: absorption lines, quasars: individual (SDSS J1001+5027)
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

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Inada, Naohisa

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Oguri, Masamune

× Oguri, Masamune

Oguri, Masamune

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Charlton, Jane C.

× Charlton, Jane C.

Charlton, Jane C.

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Eracleous, Michael

× Eracleous, Michael

Eracleous, Michael

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Koyamada, Suzuka

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Koyamada, Suzuka

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Itoh, Daisuke

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Itoh, Daisuke

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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 ASTROPHYSICAL JOURNAL.854(1):69(2018)
書誌情報 ASTROPHYSICAL JOURNAL

巻 854, 号 1, p. 69, 発行日 2018-02-10
抄録
内容記述 We performed spectroscopic observations of the small-separation lensed quasar SDSS J1001+5027, whose images have an angular separation q = 2 ''.86, and placed constraints on the physical properties of gas clouds in the vicinity of the quasar (i.e., in the outflowing wind launched from the accretion disk). The two cylinders of sight to the two lensed images go through the same region of the outflowing wind and they become fully separated with no overlap at a very large distance from the source (similar to 330 pc). We discovered a clear difference in the profile of the C IV broad absorption line (BAL) detected in the two lensed images in two observing epochs. Because the kinematic components in the BAL profile do not vary in concert, the observed variations cannot be reproduced by a simple change of ionization state. If the variability is due to gas motion around the background source (i.e., the continuum source), the corresponding rotational velocity is v(rot) >= 18,000 km s(-1), and their distance from the source is r <= 0.06 pc assuming Keplerian motion. Among three Mg II and three C IV NAL systems that we detected in the spectra, only the Mg II system at z(abs) = 0.8716 shows a hint of variability in its Mg I profile on a rest-frame timescale of Delta t(rest) <= 191. days and an obvious velocity shear between the sightlines whose physical separation is similar to 7 kpc. We interpret this as the result of motion of a cosmologically intervening absorber, perhaps located in a foreground galaxy.
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 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
権利
権利情報 © 2018. 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=000425000100009
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Cite as

Misawa, Toru, Inada, Naohisa, Oguri, Masamune, Charlton, Jane C., Eracleous, Michael, Koyamada, Suzuka, Itoh, Daisuke, 2018, Spectroscopic Observations of the Outflowing Wind in the Lensed Quasar SDSS J1001+5027: IOP PUBLISHING LTD, 69– p.

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