RADIO-EMISSION IN ACTIVE GALAXIES - THE STARBURST SCENARIO

被引：1
|
作者：
COLINA, L
PEREZOLEA, D
机构：
[1] Dpto. de Física Teórica, Universidad Autónoma, Madrid
来源：
ASTROPHYSICS AND SPACE SCIENCE | 1993年 / 205卷 / 01期
关键词：
D O I：
10.1007/BF00657963
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The origin of the radio emission in active galaxies ranging from LINERS to ultraluminous IRAS galaxies is considered under the scenario of a violent nuclear or circumnuclear starburst. The radio luminosity is explained as non-thermal radio emission generated in supernova remnants (SNRs). Implications of this scenario in terms of the radio brightness of SNRs, the supernovae rates, and their detectability are discussed.
引用
收藏
页码：99 / 105
页数：7
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