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Suzaku Observations of the Radio Galaxy 3C 33
https://jaxa.repo.nii.ac.jp/records/5055
https://jaxa.repo.nii.ac.jp/records/50554e7d0b7a-c936-49a4-80d0-1e3f4c2f27b4
名前 / ファイル | ライセンス | アクション |
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64574123.pdf (962.4 kB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Suzaku Observations of the Radio Galaxy 3C 33 | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | workshop: proceedings - galaxies: active - galaxies: jets - galaxies: individual (3C 33) - X-rays: galaxies | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
著者 |
Evans, A. Daniel
× Evans, A. Daniel× Reeves, James N.× Hardcastle, Martin J.× Kraft, Ralph P.× Lee, Julia C.× Virani, Shanil N. |
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著者所属(英) | ||||||
en | ||||||
MIT Kavli Institute for Astrophysics and Space Research | ||||||
著者所属(英) | ||||||
en | ||||||
Astrophysics Group, School of Physical and Geographical Sciences, Keele University | ||||||
著者所属(英) | ||||||
en | ||||||
School of Physics, Astronomy & Mathematics, University of Hertfordshire | ||||||
著者所属(英) | ||||||
en | ||||||
Harvard-Smithsonian Center for Astrophysics | ||||||
著者所属(英) | ||||||
en | ||||||
Harvard-Smithsonian Center for Astrophysics | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Astronomy, Yale University | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構 | |||||
出版者(英) | ||||||
出版者 | Japan Aerospace Exploration Agency (JAXA) | |||||
書誌情報 |
宇宙航空研究開発機構特別資料: en : JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H 巻 JAXA-SP-09-008E, p. 320-321, 発行日 2010-02-26 |
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会議概要(会議名, 開催地, 会期, 主催者等)(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We present results from a new 100 - ks Suzaku observation of the nearby radio galaxy 3C 33, and investigate the nature of absorption, reflection, and jet production in this source. We model the 2 - 70 keV nuclear continuum with a power law that is absorbed either through one or more layers of pc-scale neutral material, or through a modestly ionized pc-scale obscurer. The expected signatures of reflection from a neutral accretion disk are absent in 3C 33 : there is no evidence of a relativistically blurred Fe Kalpha emission line, and no Compton reflection hump above 10 keV. We discuss the implications of this for the nature of jet production in 3C 33. | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 1349-113X | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA11984031 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0064574123 | |||||
レポート番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | レポート番号: JAXA-SP-09-008E |