Probing highly obscured, self-absorbed galaxy nuclei with vibrationally excited HCN
Journal article, 2015
galaxies: active
galaxies: evolution
galaxies
galaxies: nuclei
Author
Susanne Aalto
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
S. Martin
Institut de Radioastronomie Millimétrique (IRAM)
Francesco Costagliola
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
E. Gonzalez-Alfonso
University of Alcalá
Sebastien Muller
Chalmers, Earth and Space Sciences, Onsala Space Observatory
K. Sakamoto
Academia Sinica
G. A. Fuller
University of Manchester
S. G. Burillo
Spanish National Observatory (OAN)
P. van der Werf
Leiden University
R. Neri
Institut de Radioastronomie Millimétrique (IRAM)
M. Spaans
University of Groningen
F. Combes
LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres
S. Viti
University College London (UCL)
S. Muhle
Argelander-Institut für Astronomie
L. Armus
California Institute of Technology (Caltech)
A. Evans
University of Virginia
National Radio Astronomy Observatory
E. Sturm
Max Planck Society
J. Cernicharo
Spanish National Research Council (CSIC)
C. Henkel
Max Planck Society
King Abdulaziz University
T. R. Greve
University College London (UCL)
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 584 A42Molecules as Diagnostic Tools for Active and Obscured Galaxies
Swedish Research Council (VR) (2011-4143), 2012-01-01 -- 2014-12-31.
Subject Categories (SSIF 2011)
Astronomy, Astrophysics and Cosmology
Infrastructure
Onsala Space Observatory
DOI
10.1051/0004-6361/201526410