The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud
Journal article, 2016
outflows / radio continuum: stars
stars: AGB and post-AGB / stars: winds
Author
M. A. T. Groenewegen
Royal Observatory of Belgium
Wouter Vlemmings
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
P. Marigo
University of Padua
G. C. Sloan
The University of North Carolina at Chapel Hill
Cornell University
Space Telescope Science Institute (STScI)
L. Decin
KU Leuven
M.W. Feast
South African Astronomical Observatory
University of Cape Town
S. R. Goldman
Keele University
Kay Justtanont
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
F. Kerschbaum
University of Vienna
M. Matsuura
Cardiff University
I. McDonald
University of Manchester
Hans Olofsson
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
R. Sahai
Jet Propulsion Laboratory, California Institute of Technology
J. T. van Loon
Keele University
P.R. Wood
Australian National University
A.A. Zijlstra
University of Manchester
J. Bernard-Salas
Open University
M. Boyer
University of Maryland
National Aeronautics and Space Administration (NASA)
L. Guzman-Ramirez
Leiden University
European Southern Observatory Santiago
O. C. Jones
Space Telescope Science Institute (STScI)
E. Lagadec
Observatoire de la Cote d'Azur
M. Meixner
Space Telescope Science Institute (STScI)
M.G. Rawlings
East Asian Observatory
S. Srinivasan
Academia Sinica
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 596 50- A50Subject Categories (SSIF 2011)
Astronomy, Astrophysics and Cosmology
Roots
Basic sciences
DOI
10.1051/0004-6361/201629590