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X-ray Spectral Transitions in Galactic X-ray Binaries: A Unified Picture of Hard-to-Soft Transitions in Persistent and Transient Sources
https://jaxa.repo.nii.ac.jp/records/5040
https://jaxa.repo.nii.ac.jp/records/50408602f327-0fc7-4199-b9e5-949a0f42f691
名前 / ファイル | ライセンス | アクション |
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64574108.pdf (119.1 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 | X-ray Spectral Transitions in Galactic X-ray Binaries: A Unified Picture of Hard-to-Soft Transitions in Persistent and Transient Sources | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | X-ray 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 |
Yu, Wenfei
× Yu, Wenfei× Yan, Zhen |
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著者所属(英) | ||||||
en | ||||||
Shanghai Astronomical Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
Shanghai Astronomical Observatory | ||||||
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. 290-292, 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 | Daily X-ray monitoring observations with the RXTE/ASM and the Swift/BAT provide unique insight into the long-term spectral evolution of the brightest persistent and transient X-ray binaries. The spectral state transitions seen with the RXTE/ASM and the Swift/BAT in the past few years confirm that there is a correlation between the luminosity of the hard-to-soft transition and the luminosity a source can reach in the following soft state. This correlation span over two orders of magnitude, showing persistent sources and transient sources, falling on the same empirical relation, differ in the rate-of-change of the observed X-ray luminosity. Therefore the luminosity at which a hard-to-soft transition occur can be primarily described by the rate-of-increase of the luminosity, a likely surrogate of the rate-of-increase of the mass accretion rate in the accretion flow, which appears as the dominating parameter which determines luminosity of the hard-to-soft transition. | |||||
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: AA0064574108 | |||||
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 |