Detection of Rotational CO Emission From the Red-supergiants in the Large Magellanic Cloud (2015)
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/eas/1571010
Publication URI: http://dx.doi.org/10.1051/eas/1571010
Type: Journal Article/Review
Parent Publication: EAS Publications Series