HIGH-LYING OH ABSORPTION, [C II] DEFICITS, AND EXTREME LFIR/MH2 RATIOS IN GALAXIES
Journal article, 2015
galaxies evolution
star-formation
Author
E. Gonzalez-Alfonso
University of Alcalá
J. Fischer
Naval Research Laboratory
E. Sturm
Max Planck Society
J. Gracia-Carpio
Max Planck Society
S. Veilleux
University of Maryland
M. Melendez
University of Maryland
D. Lutz
Max Planck Society
A. Poglitsch
Max Planck Society
Susanne Aalto
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
Niklas Falstad
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
H. W. W. Spoon
Cornell University
D. Farrah
Virginia Polytechnic Institute and State University
A. Blasco
University of Alcalá
C. Henkel
Max Planck Society
King Abdulaziz University
A. Contursi
Max Planck Society
A. Verma
University of Oxford
M. Spaans
University of Groningen
H. A. Smith
Harvard-Smithsonian Center for Astrophysics
M. L. N. Ashby
Harvard-Smithsonian Center for Astrophysics
S. Hailey-Dunsheath
California Institute of Technology (Caltech)
S. G. Burillo
Spanish National Observatory (OAN)
J. Martin-Pintado
Centro de Astrobiologia (CAB)
P. van der Werf
Leiden University
R. Meijerink
Leiden University
R. Genzel
Max Planck Society
Astrophysical Journal
0004-637X (ISSN) 1538-4357 (eISSN)
Vol. 800 1 1-10 69Subject Categories
Astronomy, Astrophysics and Cosmology
DOI
10.1088/0004-637X/800/1/69