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PSR B1259-63: 15 years of X-ray observations.
https://jaxa.repo.nii.ac.jp/records/4950
https://jaxa.repo.nii.ac.jp/records/4950eaf4d0bb-cbd8-458a-84c0-3a89f26e0e53
名前 / ファイル | ライセンス | アクション |
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64574018.pdf (274.1 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 | PSR B1259-63: 15 years of X-ray observations. | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | pulsars: PSR B1259-63 - X-rays: binaries - X-rays: PSR B1259-63 | |||||
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 |
内山, 泰伸
× 内山, 泰伸× 高橋, 忠幸× Chernyakova, Maria× Neronov, Andrii× Aharonian, Felix× Uchiyama, Yasunobu× Takahash, Tadayuki |
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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高エネルギー天文学研究系 | ||||||
著者所属(英) | ||||||
en | ||||||
Dublin Institute for Advanced Studies | ||||||
著者所属(英) | ||||||
en | ||||||
Integral Science Data Centre | ||||||
著者所属(英) | ||||||
en | ||||||
Dublin Institute for Advanced Studies | ||||||
著者所属(英) | ||||||
en | ||||||
SLAC National Accelerator Laboratory | ||||||
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. 48-49, 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 | PSR B1259-63 is a 48 ms radio pulsar in a highly eccentric 3.4 year orbit with a Be star SS 2883. The 2007 periastron passage was observed in unprecedented details with Suzaku, Swift, XMM-Newton and Chandra missions. We present here the results of this campaign and compare them with previous observations. With these data we are able, for the first time, to study the details of the spectral evolution of the source over a 2 months period of the passage of the pulsar close to the Be star. New data confirm the pre-periastron spectral hardening, with the photon index reaching a value smaller than 1.5. Such a behaviour can be explained within both synchrotron and IC model of the origin of the X-ray emission. Similarity of the form of rise and decay of the X-ray emission during the two disk passages and its resemblance to the radio lightcurve gives an argument in favour of the IC model. | |||||
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: AA0064574018 | |||||
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 |