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Suzaku observation of O and Ne abundances in interstellar medium of S0 galaxy, NGC 4382
https://jaxa.repo.nii.ac.jp/records/5082
https://jaxa.repo.nii.ac.jp/records/5082a41fc6f9-d216-4174-b2f5-9fee649adc8f
名前 / ファイル | ライセンス | アクション |
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64574150.pdf (177.7 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 | Suzaku observation of O and Ne abundances in interstellar medium of S0 galaxy, NGC 4382 | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | galaxies: individual (NGC 4382), galaxies: ISM, galaxies: abundances, X-rays: ISM | |||||
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 |
薙野, 綾
× 薙野, 綾× 松下, 恭子× Nagino, Ryo× Matsushita, Kyoko |
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著者所属 | ||||||
東京理科大学 | ||||||
著者所属 | ||||||
東京理科大学 | ||||||
著者所属(英) | ||||||
en | ||||||
Tokyo University of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Tokyo University of Science | ||||||
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. 388-389, 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 derived O and Ne abundances in the interstellar medium (ISM) of a relatively isolated S0 galaxy, NGC 4382, observed with the Suzaku XIS instrument, and compared the abundance pattern of O/Ne/Mg/Fe to those of ISM in elliptical galaxies. The O/Fe ratio is a factor of 2 smaller than those of ISM in elliptical galaxies, NGC 720, NGC 1399, NGC 1404 and NGC 4636, observed with Suzaku. Since O, Ne, Mg are predominantly synthesized by supernovae (SNe) II, the observed abundance pattern indicates that the contribution of SN Ia products is higher in the S0 galaxy, than those in elliptical galaxies. Our result supports that spiral galaxies have changed into S0 galaxies, since stars in spiral galaxies thought to contain more SN Ia products than those in ellipticals. | |||||
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: AA0064574150 | |||||
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 |