The magnetic fields and angular sizes of radio sources displaying synchrotron self-absorption

被引：0
|
作者：
A. V. Megn
机构：
[1] Raido Astronomy Institute of the National Academy of Sciences of the Ukraine,
来源：
Astronomy Reports | 2008年 / 52卷
关键词：
98.70.Dk; 98.70.Dk; 98.62.En; 98.62.Lv; 95.30.Gv;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
A method for estimating the magnetic-field strengths and angular sizes of radio sources displaying synchrotron self-absorption based on their observed radio spectra is considered. The method is used to derive the angular sizes of compact radio sources (components) and the magnetic fields in these regions, as well as the energy and number of relativistic electrons and the radiative power of a number of quasars and radio galaxies.
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页码：201 / 210
页数：9
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