The authors have developed a simple model of spot motions on a stellar surface, based on what has been observed on the Sun. This model is applied to RS CVn phenomenology, determining the parameters of the differential rotation and of the spot motion, in order to obtain group properties and classification criteria.
Photometric Variations and Spot Cycles in RS CVn Stars
BUSSO, Maurizio Maria;
1986
Abstract
The authors have developed a simple model of spot motions on a stellar surface, based on what has been observed on the Sun. This model is applied to RS CVn phenomenology, determining the parameters of the differential rotation and of the spot motion, in order to obtain group properties and classification criteria.File in questo prodotto:
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