ON THE RELATIONSHIP BETWEEN OPTICAL AND RADIO-EMISSION FROM ACTIVE GALACTIC NUCLEI

被引：0
|
作者：
ZENTSOVA, AS
FEDORENKO, VN
机构：
来源：
ASTRONOMICHESKII ZHURNAL | 1991年 / 68卷 / 01期
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We develop a model in which the radio emission of nuclei of Seyfert galaxies emerges in the regions of formation of their narrow emission lines, R approximately 100 pc. Gaseous clouds, producing this emission, are moving in the surrounding hot gas and induce shock waves. The latter accelerate electrons, which produce radio emission via synchrotron mechanism. The model explains an observational correlation between the radio and optical properties of Seyfert galaxies and makes some predictions on the parameters of the region R approximately 100 pc.
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页码：14 / 21
页数：8
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