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Study of the ejecta distribution in the Vela SNR with MAXI
https://jaxa.repo.nii.ac.jp/records/5293
https://jaxa.repo.nii.ac.jp/records/529385c71ddb-2ec9-4e2d-b52b-9d05b7991f25
名前 / ファイル | ライセンス | アクション |
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64306054.pdf (410.1 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 | Study of the ejecta distribution in the Vela SNR with MAXI | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | ISM : individual (Vela Supernova Remnant) - supernova remnants | |||||
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 |
山口, 弘悦
× 山口, 弘悦× 勝田, 哲× 平賀, 純子× 早藤, 麻美× 玉川, 徹× Yamaguchi, Hiroya× Katsuda, Satoru× Hiraga, Junko S.× Hayato, Asami× Tamagawa, Toru |
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著者所属 | ||||||
理化学研究所 | ||||||
著者所属 | ||||||
大阪大学 | ||||||
著者所属 | ||||||
理化学研究所 | ||||||
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 | ||||||
Institute of Physical and Chemical Research (RIKEN) | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Physical and Chemical Research (RIKEN) | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Physical and Chemical Research (RIKEN) | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Physical and Chemical Research (RIKEN) | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Physical and Chemical Research (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: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop 巻 JAXA-SP-08-014E, p. 270-273, 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 | The Vela supernova remnant (SNR) is a very ideal target for studying the detailed structure, since it has a quite large angular diameter (ca. 8 deg). In this proceeding, we first review the previous observations of several "shrapnels", the fragments of the ejecta protruding beyond the primary blast-shock front. Then, we report the preliminary results of shrapnel B with Suzaku. The elemental abundances are found to be significantly higher than the solar values for the first time, indicating the shrapnel originates from the supernova ejecta. Finally, we discuss the scientific significance of MAXI observations of the Vela SNR. The most part of the SNR has not yet been observed by the recent satellites, since it is too large to be covered with their limited exposure times. MAXI will be the first X-ray mission allowing us to study the ejecta distribution in the entire SNR as well as to search other ejecta fragments hiding inside the shell by the projection effect. Those information must become a key to solve the mechanism of the supernova explosions. | |||||
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: AA0064306054 | |||||
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 |