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Change of Cyclotron Resonance Energies of Binary X-ray Pulsar X0331+53
https://jaxa.repo.nii.ac.jp/records/5011
https://jaxa.repo.nii.ac.jp/records/5011a5d78e8b-2220-46c1-9e0d-ce939acfcc05
名前 / ファイル | ライセンス | アクション |
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64574079.pdf (206.4 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 | Change of Cyclotron Resonance Energies of Binary X-ray Pulsar X0331+53 | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | pulsars: individual(X0331+53) - X-rays: binariesKey words: | |||||
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 |
中島, 基樹
× 中島, 基樹× 三原, 建弘× 牧島, 一夫× Nakajima, Motoki× Mihara, Tatehiro× Makishima, Kazuo |
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著者所属 | ||||||
日本大学松戸歯学部 | ||||||
著者所属 | ||||||
理化学研究所 | ||||||
著者所属 | ||||||
理化学研究所 | ||||||
著者所属(英) | ||||||
en | ||||||
School of Dentistry at Matsudo, Nihon University | ||||||
著者所属(英) | ||||||
en | ||||||
Cosmic Radiation, RIKEN | ||||||
著者所属(英) | ||||||
en | ||||||
Cosmic Radiation, RIKEN | ||||||
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. 214-215, 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 | We report on the further analysis results of the cyclotron-resonance energy changes of X0331+53 (V0332+53) observed by RXTE in 2004-2005 outburst. This source is known to have the prominent fundamental cyclotron resonance, and that resonance energy increased from approximately 22 to approximately 27 keV as the source luminosity changed from 3.5 x 10(exp 38) ergs/s to 1.0 x 10(exp 38) ergs/s. Although the behavior of the fundamental resonances have been examined by several authors so far, the detailed analysis of the second cyclotron resonances were not performed due to the low statistics in higher energies. In order to reveal the behavior of the second cyclotron resonance, we have analyzed the whole 2004-2005 outburst data of X0331+53 with "flux-sorted analysis" method (Nakajima et al. 2006). As a result of our analysis, we clearly confirmed that the second cyclotron energy changed from approximately 49 to approximately 54 keV, implying a weaker fractional change as a function of the luminosity. The observed resonance energy ratio between the second and the fundamental cyclotron line was approximately 2.2 when the source was most luminous, whereas the ratio decreased to the nominal value of 2.0 at the least luminous state. The change of the resonance energy ratio may result from the different heights of the cyclotron scattering in the accretion column. | |||||
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: AA0064574079 | |||||
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 |