STARS;
ACTIVITY;
FLARES;
RADIO RADIATION;
BINARIES;
D O I:
10.1007/BF00749155
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
The variability of the radio emission of RS CVn and Algol type binaries has been observed over 70 hours by Lefevre et al. (1993). In this contribution simple model calculations are applied to discuss the relevant time scales. It is concluded that a significant fraction of the permanent radio emission of these systems is due to flare-like processes of energy release over a wide range of energies.