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Search for Exozodiacal Dust: Are Vega-like Stars Common ?
https://jaxa.repo.nii.ac.jp/records/36653
https://jaxa.repo.nii.ac.jp/records/366530e4cab8d-efa3-4e78-aaab-7c7e73ca5149
名前 / ファイル | ライセンス | アクション |
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SA4585143.pdf (272.5 kB)
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Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Search for Exozodiacal Dust: Are Vega-like Stars Common ? | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | departmental bulletin paper | |||||
著者 |
HIRAO, Takanori
× HIRAO, Takanori× MATSUO, Hiroshi× MATSUURA, Shinji× MURAKAMI, Hiroshi× NODA, Manabu× OOTSUBO, Takafumi× UENO, Munetaka |
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著者所属(英) | ||||||
en | ||||||
Graduate School of Science, Nagoya University | ||||||
著者所属(英) | ||||||
en | ||||||
National Astrononomical Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
The Institute of Space and Astronautical Science | ||||||
著者所属(英) | ||||||
en | ||||||
The Institute of Space and Astronautical Science | ||||||
著者所属(英) | ||||||
en | ||||||
Nagoya City Science Museum | ||||||
著者所属(英) | ||||||
en | ||||||
Graduate School of Science, The University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Graduate School of Arts and Science, The Univesity of Tokyo | ||||||
出版者 | ||||||
出版者 | 宇宙科学研究所 | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science | |||||
書誌情報 |
en : The Institute of Space and Astronautical Science report. S.P. : Mid- and Far-Infrared Astronomy and Future Space Mission 巻 14, p. 19-25, 発行日 2000-12 |
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抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Possible observations of Vega-like stars by the ASTRO-F and the HII/L2 3.5m space telescope are proposed. Vega-like stars are main sequence stars with mid-infrared and/or far-infrared excess. A few of these stars have been observed precisely at various wavelengths and it was found out that they tend to have hot (~300K) circumstellar dust like the zodiacal dust in our solar system and warm (~50K) dust ring around 30{50 AU from the central star. In spite of thesediscoveries, one question still remains; How many Vega-like stars are there? Mid- and far-infrared surveys by the ASTRO-F and the HII/L2 telescope will be the best ones to get the answer to this question. The ASTRO-F/FIS survey could detect `α Lyr' located at a distance of <50pc, within which roughly 150 of A-type main sequence stars exist. The HII/L2 3.5m telescope survey has the capability to detect much farther, up to 100pc. Thus, the total number of candidates will increase to as many as ~1000. | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0288-433X | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA10455137 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: SA4585143000 |