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The Onion-like Metallicity Structure of Tycho's Supernova Remnant as Revealed by Doppler Broadened X-ray Emission Lines
https://jaxa.repo.nii.ac.jp/records/4954
https://jaxa.repo.nii.ac.jp/records/4954d1f5f405-f300-4800-aecd-208928a668dc
名前 / ファイル | ライセンス | アクション |
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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 Onion-like Metallicity Structure of Tycho's Supernova Remnant as Revealed by Doppler Broadened X-ray Emission Lines | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | ISM: supernova remnants - supernovae: general - X-rays: individual (Tycho's SNR) | |||||
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 |
早藤, 麻美
× 早藤, 麻美× 玉川, 徹× 山口, 弘悦× 古澤, 彰浩× 小澤, 碧× 國枝, 秀世× 馬場, 彩× 牧島, 一夫× Hayato, Asami× Tamagawa, Toru× Yamaguchi, Hiroya× Furuzawa, Akihiro× Ozawa, Midori× Kunieda, Hideyo× Hughes, John P.× Hwang, Una× Bamba, Aya× Makishima, Kazuo |
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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 | ||||||
名古屋大学 | ||||||
著者所属 | ||||||
京都大学 | ||||||
著者所属 | ||||||
名古屋大学 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究本部 | ||||||
著者所属 | ||||||
東京大学 | ||||||
著者所属(英) | ||||||
en | ||||||
RIKEN | ||||||
著者所属(英) | ||||||
en | ||||||
RIKEN | ||||||
著者所属(英) | ||||||
en | ||||||
RIKEN | ||||||
著者所属(英) | ||||||
en | ||||||
Nagoya University | ||||||
著者所属(英) | ||||||
en | ||||||
Kyoto University | ||||||
著者所属(英) | ||||||
en | ||||||
Nagoya University | ||||||
著者所属(英) | ||||||
en | ||||||
Rutgers University | ||||||
著者所属(英) | ||||||
en | ||||||
NASA/GSFC | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA) | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tokyo | ||||||
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. 58-61, 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 have discovered a three-dimensional onion-like metallicity structure in Tychoapos;s SNR using Suzaku, in such a way that iron is more concentrated in the remnant center than intermediate-mass elements (IMEs: Si, S, Ar, and Ca). This is achieved by measuring widths of the emission lines of those elements as a function of the angular distance from the center of the remnant. We interpret our results as representing Doppler broadening caused by a line-of-sight velocity dispersion of the line-emitting ions. Applying two Gaussian models (red- and blue-shifted components) to each broadened line, we determine the expansion velocities of the IMEs and Fe as approximately 4900 km s(exp -1) and approximately 3800 km s(exp -1), respectively. Combining our results with the projected image of the SNR, we successfully construct a three-dimensional onion-like structure of the SNR. | |||||
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: AA0064574022 | |||||
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 |