WEKO3
アイテム
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Evidence of dust replenishment zone around beta Pictoris
https://jaxa.repo.nii.ac.jp/records/20605
https://jaxa.repo.nii.ac.jp/records/2060541f45170-2d56-40b7-bb72-8bfb20dff946
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 | Evidence of dust replenishment zone around beta Pictoris | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 塵補給ゾーン | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | ベータ・ピクトリス | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 太陽系 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 天文鉱物学 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 質量吸収係数 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 恒星間物質 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 珪酸塩 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 輝度 | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | dust replenishment zone | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | beta Pictoris | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | solar system | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | astromineralogy | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | mass absorption coefficient | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | interstellar matter | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | silicate | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | brightness | |||||
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 | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
その他のタイトル | ||||||
その他のタイトル | ベータ・ピクトリス近傍の塵補給ゾーンの証拠 | |||||
著者 |
片坐, 宏一
× 片坐, 宏一× 岡本, 美子× 本田, 充彦× 山下, 卓也× 尾中, 敬× 渡部, 潤一× 宮田, 隆志× 酒向, 重行× 藤吉, 拓哉× 左近, 樹× Kataza, Hirokazu× OkamotoKataza, Yoshiko× Honda, Mitsuhiko× Yamashita, Takuya× Onaka, Takashi× Watanabe, Junichi× Miyata, Takashi× Sako, Shigeyuki× Fujiyoshi, Takuya× Sakon, Itsuki |
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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 | ||||||
北里大学 一般教養部 自然科学教育センター | ||||||
著者所属 | ||||||
東京大学 理学部 天文学科 | ||||||
著者所属 | ||||||
国立天文台 ハワイ観測所 | ||||||
著者所属 | ||||||
東京大学 理学部 天文学科 | ||||||
著者所属 | ||||||
国立天文台 | ||||||
著者所属 | ||||||
東京大学 理学部附属天文学教育研究センター | ||||||
著者所属 | ||||||
東京大学 理学部附属天文学教育研究センター | ||||||
著者所属 | ||||||
国立天文台 ハワイ観測所 | ||||||
著者所属 | ||||||
東京大学 理学部 天文学科 | ||||||
著者所属(英) | ||||||
en | ||||||
Japan Aerospace Exploration Agency Institute of Space and Astronautical Science | ||||||
著者所属(英) | ||||||
en | ||||||
Kitasato University Center for Natural Sciences, College of Liberal Arts and Sciences | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tokyo Department of Astronomy, School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
National Astronomical Observatory Subaru Telescope | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tokyo Department of Astronomy, School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
National Astronomical Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tokyo Institute of Astronomy, Faculty of Science | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tokyo Institute of Astronomy, Faculty of Science | ||||||
著者所属(英) | ||||||
en | ||||||
National Astronomical Observatory Subaru Telescope | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tokyo Department of Astronomy, School of Science | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構宇宙科学研究本部 | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS) | |||||
書誌情報 |
第37回月・惑星シンポジウム en : Proceedings of the 37th ISAS Lunar and Planetary Symposium p. 103-106, 発行日 2004-02 |
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抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Beta Pictoris is a prominent Vega like star, which has a dusty disk around the central star. This disk is supposed to be a debris dust disk, which means that the dust in the disk is recently replenished. But so far, there is no observational evidence to indicate dust replenishment. Disk spectra in the N band have been observed and the spatially resolved dust features were obtained from the disk. The feature shows ring-like small dust emission around the star. This small dust has too short life time to survive around the star, existence of the small dust means on-going dust replenishment is now taking in a place at this area. This is the first direct evidence of the dust replenishment around the Vega like star. This ring like structure is planetesimal belt like an asteroid belt in the solar system. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0047898027 |