EXPLAINING THE [C II]157.7 μm DEFICIT IN LUMINOUS INFRARED GALAXIES—FIRST RESULTS FROM A HERSCHEL /PACS STUDY OF THE GOALS SAMPLE

T. Diaz-Santos (1) , L. Armus , V. Charmandaris (2) , S. Stierwalt , E. Murphy , S. Haan (3) , H. Inami (4) , S. Malhotra , R. Meijerink , G. Stacey , A. Petric , A. Evans (5) , S. Veilleux (6) , P. van Der Werf (7) , S. Lord , N. Lu , J. Howell , P. Appleton (8) , J. Mazzarella , J. Surace (9) , C. Xu (10) , B. Schulz (8) , D. Sanders , C. Bridge , B. Chan , D. Frayer (11) , K. Iwasawa (12) , J. Melbourne , E. Sturm (9)

1 UDP - Universidad Diego Portales [Santiago - Chili]
2 Observatoire de Paris
3 CSNSM - Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse
4 CRAL - Centre de Recherche Astrophysique de Lyon
5 IROC TECHNOLOGIES - iROc Technologies
6 University of Maryland [College Park]
7 Leiden Observatory [Leiden]
8 IPAC - Infrared Processing and Analysis Center
9 AUTRES
10 Department of Earth Sciences [Uppsala]
11 HNHP - Histoire naturelle de l'Homme préhistorique
12 UNIBO - Alma Mater Studiorum Università di Bologna = University of Bologna

Domaines: Physique [physics]; Astrophysique [astro-ph]

T. Diaz-Santos, L. Armus, V. Charmandaris, S. Stierwalt, E. Murphy, et al.. EXPLAINING THE [C II]157.7 μm DEFICIT IN LUMINOUS INFRARED GALAXIES—FIRST RESULTS FROM A HERSCHEL /PACS STUDY OF THE GOALS SAMPLE. The Astrophysical Journal, 2013, 774 (1), pp.68. ⟨10.1088/0004-637X/774/1/68⟩. ⟨hal-02520425⟩