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  1. 100 全学教育機構
  2. 1001 学術論文

MULTI-SIGHTLINE OBSERVATION OF NARROW ABSORPTION LINES IN LENSED QUASAR SDSS J1029+2623

http://hdl.handle.net/10091/00021878
a82cae62-ea0e-4066-8f58-60a485d03faf
名前 / ファイル ライセンス アクション
15K05020_03.pdf 15K05020_03.pdf (2.5 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 MULTI-SIGHTLINE OBSERVATION OF NARROW ABSORPTION LINES IN LENSED QUASAR SDSS J1029+2623
言語
言語 eng
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 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 109016

Misawa, Toru

Search repository
Saez, Cristian

× Saez, Cristian

WEKO 109017

Saez, Cristian

Search repository
Charlton, Jane C.

× Charlton, Jane C.

WEKO 109018

Charlton, Jane C.

Search repository
Eracleous, Michael

× Eracleous, Michael

WEKO 109019

Eracleous, Michael

Search repository
Chartas, George

× Chartas, George

WEKO 109020

Chartas, George

Search repository
Bauer, Franz E.

× Bauer, Franz E.

WEKO 109021

Bauer, Franz E.

Search repository
Inada, Naohisa

× Inada, Naohisa

WEKO 109022

Inada, Naohisa

Search repository
Uchiyama, Hisakazu

× Uchiyama, Hisakazu

WEKO 109023

Uchiyama, Hisakazu

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.825(1):25(2016)
書誌情報 ASTROPHYSICAL JOURNAL

巻 825, 号 1, p. 25, 発行日 2016-07-01
抄録
内容記述タイプ Abstract
内容記述 We exploit the widely separated images of the lensed quasar SDSS J1029+2623 (z(em) = 2.197, theta = 22.'' 5) to observe its outflowing wind through two different sightlines. We present an analysis of three observations, including two with the Subaru telescope in 2010 February and 2014 April, separated by four years, and one with the Very Large Telescope, separated from the second Subaru observation by similar to 2 months. We detect 66 narrow absorption lines (NALs), of which 24 are classified as intrinsic NALs that are physically associated with the quasar based on partial coverage analysis. The velocities of intrinsic NALs appear to cluster around values of v(ej) similar to 59,000, 43,000, and 29,000 km s(-1), which is reminiscent of filamentary structures obtained by numerical simulations. There are no common intrinsic NALs at the same redshift along the two sightlines, implying that the transverse size of the NAL absorbers should be smaller than the sightline distance between two lensed images. In addition to the NALs with large ejection velocities of v(ej) > 1000 km s(-1), we also detect broader proximity absorption lines (PALs) at za(bs) similar to z(em). The PALs are likely to arise in outflowing gas at a distance of r <= 620 pc from the central black hole with an electron density of n(e) >= 8.7 x 10(3) cm(-3). These limits are based on the assumption that the variability of the lines is due to recombination. We discuss the implications of these results on the three-dimensional structure of the 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
関連識別子
識別子タイプ DOI
関連識別子 https://doi.org/10.3847/0004-637X/825/1/25
関連名称
関連名称 10.3847/0004-637X/825/1/25
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=000381930000025
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