@inproceedings{oai:jaxa.repo.nii.ac.jp:00003019,
 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: 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, Spitzer and Herschel have started to reveal that SNe can form a significant mass of dust and molecules. The number of SNe studied so far is still limited. Moreover Spitzer and Herschel measurements have shown that multi-wavelength and monitoring observations are critical to build a comprehensive picture of dust and molecular formation in SNe. Equipped with near- to far-infrared imaging and spectroscopic instruments, the SPICA mission will enable a more fuller picture of supernovae and supernova remnants, potentially resolving if SNe can be a major source of dust in the interstellar medium of galaxies., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027042, レポート番号: JAXA-SP-17-010E},
 pages = {195--197},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {SPICA's Promise for Supernovae and Supernova Remnant Studies},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}