@inproceedings{oai:jaxa.repo.nii.ac.jp:00003031,
 author = {Lee, Ho Gyu and 尾中, 敬 and Koo, Bon Chul and Lee, Jae Joon and Lee, Ho Gyu and Onaka, Takashi and Koo, Bon Chul and Lee, Jae Joon},
 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, We have performed extensive near-infrared [Fe II] line observations of supernova remnants (SNRs) in our Galaxy and nearby galaxies using various instruments and telescopes. Here, we introduce our recent results from our unbiased [Fe II] imaging survey of the Galactic plane, near-infrared high-resolution imaging and spectroscopy of SNRs, and [Fe II] imaging observations of nearby galaxies. The corresponding strong line and continuum emissions at mid-infrared wavelength can be explored by sensitive instruments on SPICA., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027054, レポート番号: JAXA-SP-17-010E},
 pages = {253--255},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Fe II-Bright Supernova Remnants in Our Galaxy and Nearby Galaxies},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}