Luminous, pc-scale CO 6-5 emission in the obscured nucleus of NGC 1377
Journal article, 2017
galaxies: nuclei
galaxies: ISM
galaxies: individual: NGC 1377
galaxies: active
ISM: jets and outflows
ISM: molecules
Author
Susanne Aalto
Chalmers, Earth and Space Sciences, Onsala Space Observatory
Sebastien Muller
Chalmers, Earth and Space Sciences, Onsala Space Observatory
Francesco Costagliola
Chalmers, Earth and Space Sciences, Onsala Space Observatory
K. Sakamoto
Academia Sinica
J. S. Gallagher III
University of Wisconsin Madison
Niklas Falstad
Astronomy and Plasmaphysics
Sabine König
Astronomy and Plasmaphysics
K. M. Dasyra
University of Athens
K. Wada
Kagoshima University
F. Combes
LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres
S. G. Burillo
Spanish National Observatory (OAN)
L. Kristensen
Niels Bohr Institute
S. Martin
European Southern Observatory Santiago
Atacama Large Millimeter-submillimeter Array (ALMA)
Institut de Radioastronomie Millimétrique (IRAM)
P. van der Werf
Leiden University
A. S. Evans
University of Virginia
National Radio Astronomy Observatory
J. Kotilainen
University of Turku
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 608 A22- A22Molecules as Diagnostic Tools for Active and Obscured Galaxies
Swedish Research Council (VR) (2011-4143), 2012-01-01 -- 2014-12-31.
Subject Categories
Astronomy, Astrophysics and Cosmology
DOI
10.1051/0004-6361/201730650