STELLAR SURFACE MAGNETO-CONVECTION AS A SOURCE OF ASTROPHYSICAL NOISE. I. MULTI-COMPONENT PARAMETERIZATION OF ABSORPTION LINE PROFILES (2013)

First Author: Cegla H
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