@inproceedings{oai:jaxa.repo.nii.ac.jp:00003010,
 author = {Doublier, Vanessa and RemyRuyer, Aurelie and SAG2, Consortium},
 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, FIR observation of BCD galaxies with Herschel has revealed a wealth of new insights in these objects which are thought to resemble high-redshift forming galaxies. Dust and cold gas showed to be colder, in more or less quantities than expected and of uncertain origin. However, not unlike in the local universe, not all the dust or the cold gas is accounted for, making it more challenging. SPICA and its factor 10 to 100 in sensitivity will allow to image the faint extended cold gas/dusty disks in BCDGs in addition to detect faint C and O lines only marginally or not at all detected by Herschel., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027033, レポート番号: JAXA-SP-17-010E},
 pages = {145--147},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {FIR Extended Emission from Cold Gas and Dust in Blue Compact Dwarf Galaxies: the Anomalous Cases of POX 186 and UM 461},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}