Molecules as tracers of galaxy evolution: an EMIR survey I. Presentation of the data and first results
Journal article, 2011
massive
luminous infrared galaxies
seyfert-galaxies
evolution
star-formation
galaxies: evolution
hnc line emission
ISM: molecules
arp 220
abundances
interstellar-medium
nearby galaxies
galaxies: ISM
dense gas
vibrationally excited hc3n
galaxies: active
Author
Francesco Costagliola
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
Susanne Aalto
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
M. I. Rodriguez
Spanish National Research Council (CSIC)
Sebastien Muller
Chalmers, Earth and Space Sciences, Onsala Space Observatory
H. W. W. Spoon
Cornell University
S. Martin
European Southern Observatory Santiago
Miguel Angel Perez-Torres
Spanish National Research Council (CSIC)
Antxon Alberdi
Spanish National Research Council (CSIC)
Johan Lindberg
University of Copenhagen
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
Fabien Batejat
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
E. Jutte
Ruhr-Universität Bochum
P. van der Werf
Leiden University
University of Edinburgh
F. Lahuis
Leiden University
Netherlands Institute for Space Research (SRON)
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 528 A30Advanced Radio Astronomy in Europe (RADIONET-FP7)
European Commission (EC) (EC/FP7/227290), 2009-01-01 -- 2012-06-30.
Subject Categories (SSIF 2011)
Astronomy, Astrophysics and Cosmology
Roots
Basic sciences
DOI
10.1051/0004-6361/201015628