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Discovery of non-thermal X-ray emission from radio lobes of Cygnus A
https://jaxa.repo.nii.ac.jp/records/4943
https://jaxa.repo.nii.ac.jp/records/494353b3b532-bcd3-45f2-9da9-44ff2aa33d31
名前 / ファイル | ライセンス | アクション |
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64574011.pdf (267.5 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 | Discovery of non-thermal X-ray emission from radio lobes of Cygnus A | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | galaxies: individual (Cygnus A) - magnetic fields - radiation mechanisms: non-thermal - radio continuum: galaxies - X-ray: 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 |
矢治, 裕一
× 矢治, 裕一× 田代, 信× 磯部, 直樹× 紀, 基樹× 永井, 洋× 小山, 翔子× 楠瀬, 正昭× Yaji, Yuichi× Tashiro, Makoto× Isobe, Naoki× Kino, Motoki× Asada, K× Nagai, Hiroshi× Koyama, Shoko× Kusunose, Masaaki |
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著者所属 | ||||||
埼玉大学大学院理工学研究科 | ||||||
著者所属 | ||||||
埼玉大学大学院理工学研究科 | ||||||
著者所属 | ||||||
京都大学理学研究科宇宙物理学教室 | ||||||
著者所属 | ||||||
国立天文台 | ||||||
著者所属 | ||||||
国立天文台 | ||||||
著者所属 | ||||||
国立天文台 | ||||||
著者所属 | ||||||
関西学院大学理工学部物理学科 | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, Saitama University | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, Saitama University | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Astronomy, Kyoto University | ||||||
著者所属(英) | ||||||
en | ||||||
National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
Academia Sinica Institute of Astronomy and Astrophysics | ||||||
著者所属(英) | ||||||
en | ||||||
National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, School of Science and Technology, Kwansei Gakuin 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. 34-35, 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 | Using deep Chandra ACIS observation data for Cygnus A, we report the detection of non-thermal X-rays from its radio lobes surrounded by a rich intra-cluster medium (ICM). The non-thermal X-ray is considered to be produced via an inverse Compton (IC) process. The spectral energy distribution strongly suggest that the seed photon source of the IC X-rays includes both cosmic microwave background radiation and synchrotron radiation from the lobes. The derived parameters indicate significant energy density of electrons dominance in the Cygnus A lobes under the rich ICM environment. | |||||
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: AA0064574011 | |||||
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 |