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Suzaku Discovery of Two Peculiar Clumps at the South End of the Radio Arc
https://jaxa.repo.nii.ac.jp/records/4990
https://jaxa.repo.nii.ac.jp/records/4990b24eee28-65ae-4596-9a7d-05bd0a60781d
名前 / ファイル | ライセンス | アクション |
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64574058.pdf (249.0 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 Discovery of Two Peculiar Clumps at the South End of the Radio Arc | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Galaxy: center - ISM: clouds - radio continuum: ISM - X-rays: ISM | |||||
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 |
福岡, 亮輔
× 福岡, 亮輔× 小山, 勝二× 劉, 周強× 鶴, 剛× Fukuoka, Ryosuke× Koyama, Katsuji× Ryu, Syukyo G.× Tsuru, Takeshi Go |
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著者所属 | ||||||
京都大学大学院理学研究科物理学専攻 | ||||||
著者所属 | ||||||
京都大学大学院理学研究科物理学専攻 | ||||||
著者所属 | ||||||
京都大学大学院理学研究科物理学専攻 | ||||||
著者所属 | ||||||
京都大学大学院理学研究科物理学専攻 | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, Graduate School of Science, Kyoto University | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, Graduate School of Science, Kyoto University | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, Graduate School of Science, Kyoto University | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, Graduate School of Science, Kyoto 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. 158-159, 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 | Radio non-thermal filaments and diffuse X-ray emission in the 6.4 keV line from neutral irons are unique structures seen only in the Galactic center (GC) region. These features are sites of high-energy activity, and hold the clue to clarify the structure of GC. To search for a correlation of radio non-thermal filaments and 6.4 keV or any other X-ray band emission, Suzaku observed the GC region near the Radio Arc at approximately 20 min southeast of Sagittarius A(sup *). In the 18' x 18' field of view, we found a small clump in a higher energy band (4-6 keV), and a peculiar clump in the 6.4 keV line band. Both of them are located at the south end of the Radio Arc. We report on the results, and discuss the origin of these X-ray sources. | |||||
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: AA0064574058 | |||||
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 |