The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud (2016)
Attributed to:
Dust formation by supernovae and asymptotic giant branch stars
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201629590
Publication URI: http://dx.doi.org/10.1051/0004-6361/201629590
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics