Time variability of stellar coronal sources observed by EXOSAT
DOI: 10.1016/0273-1177(90)90130-R
Bibcode: 1990AdSpR..10b.125P
Schmitt, J. H. M. M.; Pallavicini, R.
Italy, Germany
Abstract
We 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.
1990
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Advances in Space Research
Exosat
1