@inproceedings{oai:jaxa.repo.nii.ac.jp:00003002,
 author = {Farra, D. and Lebouteiller, V. and Rigopoulou, D. and BernardSalas, J. and Efstathiou, A. and GonzalezAlfonso, E. and The HERUS team},
 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 study the origin of the [O I] 63, [N II] 122, [O I] 145, and [C II] 158 line deficits in z less than 0.3 Ultraluminous Infrared Galaxies, using data from Herschel. The line deficits are consistent with arising from increased quantities of dust in HII regions, but part of the [C II] deficit may arise from an additional mechanism, plausibly increased grain charging. We briefly discuss some implications from these results for SPICA., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027025, レポート番号: JAXA-SP-17-010E},
 pages = {113--115},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Far-Infrared Line Deficits in Ultraluminous Infrared Galaxies},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}