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A Truncated Disk of the Black Hole in GX 339-4 Observed with Suzaku
https://jaxa.repo.nii.ac.jp/records/5041
https://jaxa.repo.nii.ac.jp/records/50410cb2fe03-0497-4436-aaa4-7f3f173d7910
名前 / ファイル | ライセンス | アクション |
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64574109.pdf (339.6 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 | A Truncated Disk of the Black Hole in GX 339-4 Observed with Suzaku | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | workshop: proceedings -individual (GX 339-4) -X-rays: binaries | |||||
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 |
山田, 真也
× 山田, 真也× 牧島, 一夫× 上原, 悠一× 中澤, 知洋× 高橋, 弘充× 堂谷, 忠靖× 上田, 佳宏× 海老沢, 研× 久保田, あや× Yamada, Shinya× Makishima, Kazuo× Uehara, Yuuichi× Nakazawa, Kazuhiro× Takahashi, Hiromitsu× Dotani, Tadayasu× Ueda, Yoshihiro× Ebisawa, Ken× Kubota, Aya.× Gandhi, Poshak |
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著者所属 | ||||||
東京大学理学系研究科物理学専攻 | ||||||
著者所属 | ||||||
東京大学理学系研究科物理学専攻 | ||||||
著者所属 | ||||||
東京大学理学系研究科物理学専攻 | ||||||
著者所属 | ||||||
東京大学理学系研究科物理学専攻 | ||||||
著者所属 | ||||||
広島大学大学院理学研究科物理科学専攻 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究本部 | ||||||
著者所属 | ||||||
京都大学理学研究科宇宙物理学教室 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究本部 | ||||||
著者所属 | ||||||
芝浦工業大学システム工学部電子情報システム学科 | ||||||
著者所属 | ||||||
理化学研究所 | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physical Science, Hiroshima University | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA) | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, Kyoto University | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA) | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Electronic Information Systems, Shibaura Institute of Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Cosmic Radiation Laboratory, Institute of Physical and Chemical Research (RIKEN) | ||||||
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. 292-293, 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 re-analyzed the Suzaku data of the black hole binary GX 339-4, obtained in 2007 February. We observe an Fe-K emission line in the XIS spectrum, but the data do not require its extremely relativistic broadening claimed by Miller et al. (2008). Furthermore, the disk emission seen in the softest end of the continuum yields R(sub in)/ R(sub g) approximately 11, assuming a black-hole mass of 7 solar masses and a distance of 8 kpc. Thus, the disk is likely to be truncated at > 6 R(sub g), and hence the Suzaku data can be fully explained in terms of a non-rapidly-spinning black hole (Yamada, Makishima et al. 2009, ApJL, submitted). The above results were obtained using the XIS, HXD-PIN, and HXD-GSO data covering 0.5-300 keV, in which the XIS data were carefully corrected for event pile-up effects and telemetry saturation. The source was found in the "Very High" state, with a 0.5-200 keV luminosity of 3.8 x 10(sup 38) erg/s/cm(sup 2). We successfully reproduced the wide-band spectrum as a combination of a power-law with gamma approximately 2.6, a disk blackbody with T(sub in) approximately 0.7 keV, a narrow iron line with an EW approximately 40 eV, and a reflection with Omega / 2 pi approximately 0.6. In short, we need a particular caution in quoting a disk penetration down to approximately R(sub g). | |||||
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: AA0064574109 | |||||
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 |