ALMA observations of anisotropic dust mass loss in the inner circumstellar environment of the red supergiant VY Canis Majoris
Journal article, 2015
Extended Atmosphere
circumstellar matter
evolution
Line
star outflows
Late-Type Stars
supergiants
star winds
Kinematics
Convection
3-Dimensional Morphology
Evolved
VY CMa
Submillimeter
Mu-M
Author
Eamon O Gorman
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
Wouter Vlemmings
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
A. M. S. Richards
University of Manchester
A. Baudry
Centre national de la recherche scientifique (CNRS)
Laboratoire d'Astrophysique de Bordeaux
Elvire De Beck
Chalmers, Earth and Space Sciences, Onsala Space Observatory
L. Decin
KU Leuven
G. M. Harper
Trinity College Dublin
E. M. Humphreys
European Southern Observatory (ESO)
P. Kervella
Paris Diderot University
Institut National des Sciences de l'Univers
University of Chile (UCH)
T. Khouri
Anton Pannekoek Institute for Astronomy
Sebastien Muller
Chalmers, Earth and Space Sciences, Onsala Space Observatory
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 573 Article no. L1- L1Magnetic fields and the outflows during the formation and evolution of stars (OUTFLOWMAGN)
European Commission (EC) (EC/FP7/614264), 2014-05-01 -- 2019-04-30.
Subject Categories
Astronomy, Astrophysics and Cosmology
DOI
10.1051/0004-6361/201425101