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SUZAKU Observation of 3EG J1234-1318: Gamma-Ray Emission from Forming Galaxy Clusters?
https://jaxa.repo.nii.ac.jp/records/4961
https://jaxa.repo.nii.ac.jp/records/49612e5060fb-f732-4dff-b180-01b2fd85d39c
名前 / ファイル | ライセンス | アクション |
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64574029.pdf (214.7 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 Observation of 3EG J1234-1318: Gamma-Ray Emission from Forming Galaxy Clusters? | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | X-rays: gamma-rays: galaxies: clusters: non-thermal | |||||
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 |
真喜屋, 龍
× 真喜屋, 龍× 戸谷, 友則× 中澤, 知洋× Makiya, Ryu× Totani, Tomonori× Nakazawa, Kazuhiro |
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著者所属 | ||||||
京都大学理学研究科宇宙物理学教室 | ||||||
著者所属 | ||||||
京都大学理学研究科宇宙物理学教室 | ||||||
著者所属 | ||||||
東京大学理学系研究科物理学専攻 | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Astronomy, Kyoto University | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Astronomy, Kyoto University | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, Tokyo 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. 86-87, 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 report a SUZAKU observation of an unidentified EGRET source 3EG J1234-1318. In the region around 3EGJ1234-1318 there are several galaxy clusters and filamentary structures connecting them, and non-thermal emission via the inverse-Compton mechanism with electrons accelerated by shocks produced in structure formation and CMB photons may be the origin of the 3EGJ1234-1318. We observed 3EGJ1234-1318 in Dec. 2006 and Dec. 2007. Non-thermal diffuse emission is not detected significantly, so we derived a flux upper limit and obtain a lower limit of the size of the non-thermal emission region, which is about twice of the size of the filamentary structure. | |||||
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: AA0064574029 | |||||
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 |