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Swift Observations of the Ultraluminous X-ray Source Holmberg IX X-1
https://jaxa.repo.nii.ac.jp/records/5044
https://jaxa.repo.nii.ac.jp/records/504458b075a2-70f0-4954-9f0f-5e94ce86f02f
名前 / ファイル | ライセンス | アクション |
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64574112.pdf (146.8 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 | Swift Observations of the Ultraluminous X-ray Source Holmberg IX X-1 | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | accretion, accretion disks - binaries: close - stars: individual: Holmberg IX X-1 - X-rays: black holes - 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 |
Kong, A.K.H.
× Kong, A.K.H.× Yang, Y.-J.× Yen, T.-C. |
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著者所属(英) | ||||||
en | ||||||
Institute of Astronomy, National Tsing Hua University | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Astronomy, National Tsing Hua University | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Astronomy, National Tsing Hua 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. 298-299, 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 | Holmberg IX X-1 is a well-known ultraluminous X-ray source with an X-ray luminosity of approximately 10(exp 40) erg s(sup -1). The source has been monitored by the X-ray Telescope of Swift regularly. Since 2009 April, the source has been in an extended low luminosity state. We utilize the co-added spectra taken at different luminosity states to study the spectral behavior of the source. The best overall fits are provided by a dual thermal model with a cool blackbody and a warm disk blackbody. This suggests that Holmberg IX X-1 may be a stellar-mass black hole accreting at or above the Eddington limit and we are observing both the inner regions of the accretion disk and outflows from the compact object. | |||||
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: AA0064574112 | |||||
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 |