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The absorption structures in spectra of 1E1207.4-5409 seen by Suzaku
https://jaxa.repo.nii.ac.jp/records/5012
https://jaxa.repo.nii.ac.jp/records/501212f93b91-9155-4ba7-966c-57e8d7be5475
名前 / ファイル | ライセンス | アクション |
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64574080.pdf (236.1 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 | The absorption structures in spectra of 1E1207.4-5409 seen by Suzaku | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Pulsars: individual (1E1207.4-5209) - Stars: neutron | |||||
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 |
吉田, 篤正
× 吉田, 篤正× 杉田, 聡司× 山岡, 和貴× 中川, 友進× Takahashi, Ichiro× Yoshida, Atsumasa× Sugita, Satoshi× Kojima, Toru× Yamaoka, Kazutaka× Nakagawa, Yujin E. |
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著者所属 | ||||||
青山学院大学 | ||||||
著者所属 | ||||||
青山学院大学 | ||||||
著者所属 | ||||||
青山学院大学 | ||||||
著者所属 | ||||||
青山学院大学 | ||||||
著者所属 | ||||||
青山学院大学 | ||||||
著者所属 | ||||||
理化学研究所 | ||||||
著者所属(英) | ||||||
en | ||||||
Aoyama Gakuin University | ||||||
著者所属(英) | ||||||
en | ||||||
Aoyama Gakuin University | ||||||
著者所属(英) | ||||||
en | ||||||
Aoyama Gakuin University | ||||||
著者所属(英) | ||||||
en | ||||||
Aoyama Gakuin University | ||||||
著者所属(英) | ||||||
en | ||||||
Aoyama Gakuin University | ||||||
著者所属(英) | ||||||
en | ||||||
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. 216-217, 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 observed the strange X-ray "pulsar" 1E1207.4-5409 using Suzaku and investigated its spectral structures. 1E1207.4-5409 is an X-ray source near the center of the SNR G296.5 + 10.0. Soft X-ray observations by Chandra and XMM-Newton reported "harmonic" absorption structures at about 0.7, 1.4, and 2.1 keV (also might be at around 2.8 keV) in the energy spectrum (Bigmani et al. 2003, Luca et al.2004). The origin of these structures has not clarified yet. If these structures could be due to proton-cyclotron resonance, the magnetic field should be in the range of B approximately 10(exp 14) G, and it would serve as a strong support for the existence of magnetar. Suzaku made observations of this strange source twice and obtained spectral data displaying similar absorption structures at about 0.7, 1.4 and 2.1 keV. | |||||
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: AA0064574080 | |||||
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 |