宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)
宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)
Durham University
University of Denver
University of Denver
東京大学
国立天文台岡山天体物理観測所
European Space Astronomy Centre, European Space Agency (ESAC/ESA)
著者所属(英)
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)
Durham University
University of Denver
University of Denver
The University of Tokyo
Okayama Astrophysical Observatory, National Astronomical Observatory of Japan
European Space Astronomy Centre, European Space Agency (ESAC/ESA)
出版者
宇宙航空研究開発機構(JAXA)
出版者(英)
Japan Aerospace Exploration Agency (JAXA)
雑誌名
宇宙航空研究開発機構特別資料
雑誌名(英)
JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe
巻
JAXA-SP-17-010E
ページ
269 - 271
発行年
2018-03-09
会議概要(会議名, 開催地, 会期, 主催者等)(英)
SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan
抄録(英)
Results of infrared photometries and dust shell modeling of a peculiar object WISE J180956.27-330500.2 are presented. The object has shown a significant time variation of its SED in the last 30 years. The variation is understood as a formation and expansion of massive dust shell since late 1990’s. The object was suspected to be a red star in the optical wavelengths before the mass ejection, which allows us to hypothesize that the object is possibly the first example of the AGB star just experiencing an episodic mass loss after a thermal pulse. Observation of this object with SPICA after some 10 years from now will bring us an important clue to understand the stellar evolution and mass loss, as well as the chemistry in the thick circumstellar envelopes.
内容記述
形態: カラー図版あり
内容記述(英)
Physical characteristics: Original contains color illustrations