Explaining the [C II]157.7 μm deficit in luminous infrared galaxies—first 
results from a Herschel/PACS study of the GOALS sample

Díaz-Santos, T.; Armus, L.; Charmandaris, V.; Stierwalt, S.; Murphy, E. J.; Haan, S.; Inami, H.; Malhotra, S.; Meijerink, R.; Stacey, G.; Petric, A. O.; Evans, A. S.; Veilleux, S.; van der Werf, P. P.; Lord, S.; Lu, N.; Howell, J. H.; Appleton, P.; Mazzarella, J. M.; Surace, J. A.; Xu, C. K.; Schulz, B.; Sanders, D. B.; Bridge, C.; Chan, B. H. P.; Frayer, D. T.; Iwasawa, K.; Melbourne, J.; Sturm, E.

doi:10.1088/0004-637X/774/1/68

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Explaining the [C II]157.7 μm deficit in luminous infrared galaxies—first results from a Herschel/PACS study of the GOALS sample

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Sturm, E.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Díaz-Santos, T., Armus, L., Charmandaris, V., Stierwalt, S., Murphy, E. J., Haan, S., et al. (2013). 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, 774(1): 68, pp. 1-13. doi:10.1088/0004-637X/774/1/68.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0014-6928-5

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