VARIABILITY AND ORIGIN OF PERMANENT RADIO-EMISSION IN RS CVN AND ALGOL-TYPE BINARIES

被引:3
作者
LEFEVRE, E
KLEIN, KL
LESTRADE, JF
机构
[1] Section de Meudon, Observatoire de Paris, Meudon
关键词
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.
引用
收藏
页码:293 / 296
页数:4
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