@inproceedings{oai:jaxa.repo.nii.ac.jp:00003100,
 author = {松浦, 美香子 and Matsuura, Mikako},
 book = {宇宙航空研究開発機構特別資料, JAXA Special Publication: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life},
 month = {Mar},
 note = {第4回「あかり」国際会議 (2017年10月17-20日. 東京大学), 文京区, 東京, The 4th AKARI International Conference: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life (October 17-20, 2017. The University of Tokyo), Bunkyo-ku, Tokyo, Japan, This proceeding presents the progress of our understanding of asymptotic giant branch (AGB) stars and supernovae (SNe) made by the AKARI, the Spitzer Space Telescope, the Herschel Space Observatory and Stratospheric Observatory For Infrared Astronomy (SOFIA). The AKARI and Spitzer surveys mapped the spatial distributions of asymptotic giant branch (AGB) stars in the Milky Way and Magellanic Clouds. The survey captured how much gas and dust have been returned from AGB stars into the interstellar medium (ISM). While dust return from AGB stars has been well established, dust return from high-mass stars had not been well studied. AKARI and Spitzer opened up new insight of dust condensation in the ejecta of supernovae, as well as possible dust destruction process. Finally, prospects of the research field will be discussed with future infrared space missions, the JWST and the SPICA., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730026026, レポート番号: JAXA-SP-17-009E},
 pages = {161--165},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Infrared studies of AGB stars and supernovae with AKARI and future space missions},
 volume = {JAXA-SP-17-009E},
 year = {2018}
}