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Time variability of stellar coronal sources observed by EXOSAT

R. Pallavicini - No affiliation found

1990/01/01 Full-length article DOI: 10.1016/0273-1177(90)90130-R Journal: Advances in Space Research

Abstract:

AbstractWe present an overview of time variability in stellar coronal sources as observed with the EXOSAT satellite. We focus on M dwarf flare stars and we discuss both quiescent and flaring emission. We also outline recent developments in the modelling of stellar flares.