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Thermal Radiation from Pulsars
https://jaxa.repo.nii.ac.jp/records/4993
https://jaxa.repo.nii.ac.jp/records/49939b94d192-599e-4345-bcda-34971f75c51b
名前 / ファイル | ライセンス | アクション |
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64574061.pdf (208.4 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 | Thermal Radiation from Pulsars | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | neutron stars: pulsars | |||||
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 |
Tsuruta, Sachiko
× Tsuruta, Sachiko |
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著者所属(英) | ||||||
en | ||||||
Physics Department, Montana State 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. 166-169, 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 | Since the first detection of thermal radiation directly from the stellar surface of four pulsars by ROSAT, number of pulsars with detected thermal radiation has increased significantly. By carefully analyzing the data and comparing the results with thermal evolution theories, we now have realistic hope for exploring the composition of ultrahigh density matter. Currently, the data of Vela pulsar already suggest that the core of high mass neutron stars should include such exotic particles as hyperons and/or pion condensates. However, to confirm such possibilities, more such data for more pulsars are badly needed. Fortunately, it was found recently that soft X-ray transients (SXT) in low-mass X-ray binaries (LMXB) can provide additional such extra data when they are in quiescence. Moreover, these data helped us better understand the composition of neutron star crusts and atmospheres also. We will summarize these developments, and emphasize that future observatories such as ASTRO-H and IXO will mean breakthroughs in this exciting area. | |||||
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: AA0064574061 | |||||
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 |