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Broadband X-Ray Spectroscopy of A0535+262 with Suzaku
https://sucra.repo.nii.ac.jp/records/13278
https://sucra.repo.nii.ac.jp/records/13278dc6febd6-d4d7-4ea1-9ce7-91caae79c088
名前 / ファイル | ライセンス | アクション |
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A1002699.pdf (393.3 kB)
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Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2008-06-05 | |||||
タイトル | ||||||
タイトル | Broadband X-Ray Spectroscopy of A0535+262 with Suzaku | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | pulsars : individual (A0535+262) | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | stars : neutron | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | X-rays : stars | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | journal article | |||||
著者 |
Naik, S.
× Naik, S.× Dotani, T.× 寺田, 幸功× Nakajima, M.× Mihara, T.× Suzuki, M.× Makishima, K.× Sudoh, K.× Kitamoto, S.× Nagase, F.× Enoto, T.× Takahashi, H. |
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著者 ローマ字 | ||||||
Naik, S. | ||||||
著者 ローマ字 | ||||||
Dotani, T. | ||||||
著者 ローマ字 | ||||||
Terada, Yukikatsu | ||||||
著者 ローマ字 | ||||||
Nakajima, M. | ||||||
著者 ローマ字 | ||||||
Mihara, T. | ||||||
著者 ローマ字 | ||||||
Suzuki, M. | ||||||
著者 ローマ字 | ||||||
Makishima, K. | ||||||
著者 ローマ字 | ||||||
Sudoh, K. | ||||||
著者 ローマ字 | ||||||
Kitamoto, S. | ||||||
著者 ローマ字 | ||||||
Nagase, F. | ||||||
著者 ローマ字 | ||||||
Enoto, T. | ||||||
著者 ローマ字 | ||||||
Takahashi, H. | ||||||
著者 所属 | ||||||
著者 所属 | ||||||
著者 所属 | ||||||
独立行政法人理化学研究所中央研究所宇宙放射線研究室(現 : 埼玉大学大学院理工学研究科物質科学部門) | ||||||
著者 所属(別言語) | ||||||
著者 所属(別言語) | ||||||
著者 所属(別言語) | ||||||
Cosmic Radiationn Laboratory, The Institute of Physics and Chemical Research (RIKEN)(Present : Graduate School of Science and Engineering, Saitama University) | ||||||
書誌情報 |
Astrophysical Journal 巻 672, 号 1, p. 516-523, 発行日 2008 |
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年月次 | ||||||
2008-1 | ||||||
出版者名 | ||||||
出版者 | American Astronomical Society | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0004637X | |||||
DOI | ||||||
関連タイプ | isVersionOf | |||||
識別子タイプ | DOI | |||||
関連識別子 | info:doi/10.1086/523295 | |||||
抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | The transient X-ray binary pulsar A0535+262 was observed with Suzaku on 2005 September 14 when the source was in the declining phase of the August-September minor outburst. The similar to 103 s X-ray pulse profile was strongly energy dependent, with a double-peaked profile in the soft X-ray energy band (< 3 keV) and a single-peaked smooth profile in hard X-rays. The width of the primary dip is found to increase with energy. The broadband energy spectrum of the pulsar is well described with a negative and positive power law with exponential (NPEX) continuum model, along with a blackbody component for soft excess. A weak iron K alpha emission line with an equivalent width similar to 25 eV was detected in the source spectrum. The blackbody component is found to be pulsating over the pulse phase, implying that the accretion column and/or the inner edge of the accretion disk may be the possible emission site of the soft excess in A0535+262. The higher value of the column density is believed to be the cause of the secondary dip in the soft X-ray energy band. The iron line equivalent width is found to be constant (within errors) over the pulse phase. However, a sinusoidal type of flux variation of the iron emission line, in phase with the hard X-ray flux, suggests that the inner accretion disk is the possible emission region of the iron fluorescence line. | |||||
注記 | ||||||
内容記述タイプ | Other | |||||
内容記述 | http://www.journals.uchicago.edu/doi/abs/10.1086/523295 | |||||
版 | ||||||
[著者版] | ||||||
著者版フラグ | ||||||
出版タイプ | AM | |||||
出版タイプResource | http://purl.org/coar/version/c_ab4af688f83e57aa | |||||
資源タイプ | ||||||
内容記述タイプ | Other | |||||
内容記述 | text | |||||
フォーマット | ||||||
内容記述タイプ | Other | |||||
内容記述 | application/pdf | |||||
作成日 | ||||||
日付 | 2008-06-05 | |||||
日付タイプ | Created | |||||
アイテムID | ||||||
A1002699 |