CAN WE PREDICT THE GLOBAL MAGNETIC TOPOLOGY OF A PRE-MAIN-SEQUENCE STAR FROM ITS POSITION IN THE HERTZSPRUNG-RUSSELL DIAGRAM? (2012)
Attributed to:
Astrophysics at St Andrews: 2012-2014
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1088/0004-637x/755/2/97
Publication URI: http://dx.doi.org/10.1088/0004-637x/755/2/97
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2
ISSN: 0004-637X