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.
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页码：99 / 105
页数：7
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