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Suzaku observation of AXP 1E 1841-045 and the future observation in the MAXI era
https://jaxa.repo.nii.ac.jp/records/5263
https://jaxa.repo.nii.ac.jp/records/5263c931c1d3-472b-4a6b-a61b-4fd7af46264f
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
64306024.pdf (592.0 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 | ||||||||||
| タイトル | Suzaku observation of AXP 1E 1841-045 and the future observation in the MAXI era | |||||||||
| 言語 | en | |||||||||
| 言語 | ||||||||||
| 言語 | eng | |||||||||
| キーワード | ||||||||||
| 言語 | en | |||||||||
| 主題Scheme | Other | |||||||||
| 主題 | workshop : proceedings - LaTeX2.09 : style file - instructions | |||||||||
| 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 |
森井, 幹雄
× 森井, 幹雄
× Morii, Mikio
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| 著者所属 | ||||||||||
| 立教大学 | ||||||||||
| 著者所属（英） | ||||||||||
| en | ||||||||||
| Rikkyo University | ||||||||||
| 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: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop 巻 JAXA-SP-08-014E, p. 114-119, 発行日 2009-02-27 |
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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 | Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008) | |||||||||
| 抄録（英） | ||||||||||
| 内容記述タイプ | Other | |||||||||
| 内容記述 | We report results of the Suzaku observation of the anomalous X-ray pulsar (AXP) 1E 1841-045. We obtained the spectrum from 0.4 keV to ca. 70 keV simultaneously. The model consisting of a blackbody and two power-law functions could simulate the spectrum well. We also found that the power-law function at the higher energy can be replaced with a thermal bremsstrahlung. The fact that the hard X-ray emission can be interpreted as a thermal bremsstrahlung would support the theoretical emission model proposed by Thompson & Beloborodov (2005). Emission mechanism of the hard X-ray component can be understood by detecting the variability of the photon index and cutoff energy. In this reason, the MAXI monitoring for magnetars (AXPs and SGRs) are extremely important. The monitoring of the pulse frequency and pulse profiles of magnetars are also important as well as that of the flux. MAXI can detect transient phenomena and trigger the multi-wavelength observation. Especially, near-infrared monitoring observation and correlation study would be able to elucidate the mysterious infrared emission mechanism of magnetars. We estimated the detectability of the magnetars and their pulsation by MAXI using the MAXI simulator. | |||||||||
| 内容記述（英） | ||||||||||
| 内容記述タイプ | Other | |||||||||
| 内容記述 | Physical characteristics: Original contains color illustrations | |||||||||
| 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: AA0064306024 | |||||||||
| 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-08-014E | |||||||||
