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Search for Sc-K Line Emission from RX J0852.0-4622 Supernova Remnant with Suzaku
https://sucra.repo.nii.ac.jp/records/13443
https://sucra.repo.nii.ac.jp/records/134434b22cdb3-83c0-4c42-b5e7-3b9b86e8696f
名前 / ファイル | ライセンス | アクション |
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A1002909.pdf (475.4 kB)
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Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2009-07-13 | |||||
タイトル | ||||||
タイトル | Search for Sc-K Line Emission from RX J0852.0-4622 Supernova Remnant with Suzaku | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | ISM: supernova remnant | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | X-ray: individual [RX J0852.0-4622 (Vela Jr.)] | |||||
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 |
Hiraga, Junko S.
× Hiraga, Junko S.× Kobayashi, Yusuke× Tamagawa, Toru× Hayato, Asami× Bamba, Aya× 寺田, 幸功× Petre, Robert× Katagiri, Hideaki× Tsunemi, Hiroshi |
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著者 ローマ字 | ||||||
Hiraga, Junko S. | ||||||
著者 ローマ字 | ||||||
Kobayashi, Yusuke | ||||||
著者 ローマ字 | ||||||
Tamagawa, Toru | ||||||
著者 ローマ字 | ||||||
Hayato, Asami | ||||||
著者 ローマ字 | ||||||
Bamba, Aya | ||||||
著者 ローマ字 | ||||||
Terada, Yukikatsu | ||||||
著者 ローマ字 | ||||||
Petre, Robert | ||||||
著者 ローマ字 | ||||||
Katagiri, Hideaki | ||||||
著者 ローマ字 | ||||||
Tsunemi, Hiroshi | ||||||
著者 所属 | ||||||
著者 所属 | ||||||
著者 所属 | ||||||
著者 所属 | ||||||
著者 所属 | ||||||
著者 所属 | ||||||
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) | ||||||
著者 所属(別言語) | ||||||
著者 所属(別言語) | ||||||
著者 所属(別言語) | ||||||
Graduate School of Science and Engineering, Saitama University | ||||||
書誌情報 |
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 巻 61, 号 2, p. 275-281, 発行日 2009 |
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年月次 | ||||||
2009 | ||||||
出版者名 | ||||||
出版者 | Astronomical Society of Japan | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 00046264 | |||||
抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | We searched for evidence of line emission around 4 keV from the northwestern rim of the supernova remnant RX J0852.0-4622 using Suzaku XIS data. Several papers have reported on the detection of an emission line around 4.1 keV from this region of the sky. This line Would arise from K-band fluorescence by Sc-44, the immediate decay product of Ti-44. We performed spectral analysis for the entire portion of the NW rim of the remnant within the XIS field of view, as well as various regions corresponding to regions of published claims of line emission. We found no line emission around 4.1 keV anywhere, and are able to set a restrictive Upper limit to the X-ray flux: 1.1 x 10(-6) s(-1) cm(-2) for the entire field. For every region, our flux upper limit falls below that of the previously claimed detection. Therefore, we conclude that, to date, no definite X-ray line feature from Sc-K emission has been detected in the NW rim of RX J0852.0-4622. Our negative-detection supports the recent claim that RX J0852-4622 is neither young (1700-4000 yr) nor nearby (similar to 750 pc). | |||||
注記 | ||||||
内容記述タイプ | Other | |||||
内容記述 | arXiv:0906.0216v1 [astro-ph.HE] http://arxiv.org/abs/0906.0216/ | |||||
版 | ||||||
[出版社版] | ||||||
著者版フラグ | ||||||
出版タイプ | VoR | |||||
出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
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 | 2009-07-13 | |||||
日付タイプ | Created | |||||
アイテムID | ||||||
A1002909 |