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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. 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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 \u003c45 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."}]}, "item_6_textarea_68": {"attribute_name": "wosonly abstract", "attribute_value_mlt": [{"subitem_textarea_value": "galaxies: evolution; galaxies: formation; intergalactic medium; quasars: absorption lines; X-rays: galaxies"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Chartas, G."}], "nameIdentifiers": [{"nameIdentifier": "109024", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Cappi, M."}], "nameIdentifiers": [{"nameIdentifier": "109025", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Hamann, F."}], "nameIdentifiers": [{"nameIdentifier": "109026", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Eracleous, M."}], "nameIdentifiers": [{"nameIdentifier": "109027", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Strickland, S."}], "nameIdentifiers": [{"nameIdentifier": "109028", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Giustini, M."}], "nameIdentifiers": [{"nameIdentifier": "109029", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Misawa, T."}], "nameIdentifiers": [{"nameIdentifier": "109030", "nameIdentifierScheme": "WEKO"}]}]}, "item_files": {"attribute_name": "ファイル情報", "attribute_type": "file", "attribute_value_mlt": [{"accessrole": "open_date", "date": [{"dateType": "Available", "dateValue": "2020-02-28"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "15K05020_04.pdf", "filesize": [{"value": "1.4 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensefree": "© 2016. 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THE WIDE-ANGLE OUTFLOW OF THE LENSED z=1.51 AGN HS 0810+2554
http://hdl.handle.net/10091/00021879
http://hdl.handle.net/10091/0002187961142be2-3d2a-4bbc-8eb4-a2b6889e1fb7
名前 / ファイル | ライセンス | アクション |
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Item type | 学術雑誌論文 / Journal Article(1) | |||||
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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.× Cappi, M.× Hamann, F.× Eracleous, M.× Strickland, S.× Giustini, M.× Misawa, T. |
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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 |
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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 |