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Suzaku Observations of Accreting White Dwarfs
https://jaxa.repo.nii.ac.jp/records/4995
https://jaxa.repo.nii.ac.jp/records/4995dc87f6c8-3d6d-44a5-8729-39e38bf1902f
名前 / ファイル | ライセンス | アクション |
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64574063.pdf (466.5 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 Observations of Accreting White Dwarfs | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | stars: cataclysmic variables - X-rays: stars | |||||
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 |
石田, 学
× 石田, 学× Ishida, Manabu |
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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(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA) | ||||||
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. 174-177, 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 | Results from Suzaku observations on accreting white dwarfs are reviewed comprehensively. Suzaku identified the nova V458 Vul as an ONe-nova from X-ray spectroscopy with the XIS, which demonstrates Suzaku capability of understanding the nature of novae. Initial results on detection of a power-law component from the polar AM Her in its low state are reported. High spectral resolution and wide energy band of the XIS and the HXD enable us to determine the mass of white dwarfs in intermediate polars with unprecedented accuracy. Recently, some 80 % of the galactic ridge X-ray emission is resolved into point sources. Based on luminosity distribution and space density, we consider non-magnetic CVs as the major contributor to the galactic ridge X-ray emission. | |||||
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: AA0064574063 | |||||
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 |