STELLAR SURFACE MAGNETO-CONVECTION AS A SOURCE OF ASTROPHYSICAL NOISE. I. MULTI-COMPONENT PARAMETERIZATION OF ABSORPTION LINE PROFILES (2013)
Attributed to:
The transient sky: an integrated programme of study 2011 - 2016
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1088/0004-637x/763/2/95
Publication URI: http://dx.doi.org/10.1088/0004-637x/763/2/95
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2
ISSN: 0004-637X