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The Suzaku view of the BLRG 3C 111
https://jaxa.repo.nii.ac.jp/records/5064
https://jaxa.repo.nii.ac.jp/records/5064b0342848-190f-41b7-8c5b-e3c8093a7512
名前 / ファイル | ライセンス | アクション |
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64574132.pdf (317.4 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 | The Suzaku view of the BLRG 3C 111 | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | workshop: proceedings - galaxies: active - galaxies: individual: 3C 111 - galaxies: nuclei - 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 |
Ballo, Lucia
× Ballo, Lucia× Sambruna, Rita× Braito, Valentina× Reeves, James N.× Tavecchio, Fabrizio |
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著者所属(英) | ||||||
en | ||||||
IFCA (CSIC-UC) | ||||||
著者所属(英) | ||||||
en | ||||||
NASA/GSFC, Code 661 | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics & AstronomyUniversity of Leicester | ||||||
著者所属(英) | ||||||
en | ||||||
Astrophysics Group, School of Physical & Geographical Sciences, Keele University | ||||||
著者所属(英) | ||||||
en | ||||||
INAF - Osservatorio Astronomico di Brera | ||||||
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. 338-339, 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 | Here we report on a Suzaku observation of the nearby BLRG 3C 111, a bright FR II with a single sided jet exhibiting superluminal motion. Preliminary results indicate that the 0.5 - 200 keV spectrum is dominated by a disklike component, with a power law with photon index approximately 1.6 cutting off around 100 keV, and a reflection R approximately 0.04. The Suzaku data do not indicate the presence of a hard X-ray component associated with the jet emission, that should become dominant at GeV energies (i.e. in the range covered by FERMI ). | |||||
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: AA0064574132 | |||||
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 |