@inproceedings{oai:jaxa.repo.nii.ac.jp:00003018,
 author = {左近, 樹 and 尾中, 敬 and 田中, 雅臣 and 野沢, 貴也 and 大澤, 亮 and 片坐, 宏一 and Kemper, Ciska and Sakon, Itsuki and Onaka, Takashi and Tanaka, Masaomi and Nozawa, Takaya and Ohsawa, Ryou and Kataza, Hirokazu and Kemper, Ciska},
 book = {宇宙航空研究開発機構特別資料, JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe},
 month = {Mar},
 note = {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, In this article, some key science cases of SPICA are discussed focusing on (1) the dust formation associated with mass loss activities of evolved massive stars (e.g., Wolf-Rayet stars) before the SN explosion and (2) the dust formation in the ejecta of SNe and its evolution (destruction and/or grain growth) in a timescale of a few - a few tens years from its synthesis., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027041, レポート番号: JAXA-SP-17-010E},
 pages = {191--194},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Understanding the Role of Massive Stars on the Dusty ISM Environment in Galaxies with SPICA},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}