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.
Time variability of stellar coronal sources observed by EXOSAT
Advances in Space Research ; 10 , 2 ; 125-128
1989-01-01
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Elsevier | 1989
|EXOSAT observations of two gamma-ray burst sources
Elsevier | 1986
|European X-ray observatory satellite (Exosat)
NTRS | 1983
Tema Archiv | 1981
|