@inproceedings{oai:jaxa.repo.nii.ac.jp:00003016,
 author = {Madden, Suzanne C. and RemyRuyer, Aurelie and Cormier, Diane and Lebouteiller, Vianney and Galliano, Frederic and The PACS teams and SPIRE GT teams},
 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, Herschel has brought new light on the structure and properties of the gas and dust in low metallicity galaxies. The sensitivity of SPICA will leap beyond Herschel to revolutionise this study, where crucial observational constraints on the dust and gas properties of the extremely low metallicity galaxies has been lacking. We review our current knowledge of the low metallicity dust and gas properties in terms of where Herschel and Spitzer have brought us and how SPICA will go even further in this field., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027039, レポート番号: JAXA-SP-17-010E},
 pages = {179--183},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {The Properties and the Structure of the ISM of Low Metallicity Dwarf Galaxies: From Herschel to SPICA},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}