HOT HORIZONTAL BRANCH STARS IN ? CENTAURI: CLUES ABOUT THEIR ORIGIN FROM THE CLUSTER COLOR MAGNITUDE DIAGRAM (2009)
Attributed to:
Astrophysics Research at Liverpool John Moores University
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1088/0004-637x/702/2/1530
Publication URI: http://dx.doi.org/10.1088/0004-637x/702/2/1530
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2
ISSN: 0004-637X