Physical conditions in faint gigahertz-peaked spectrum radio sources

被引:0
|
作者
S. A. Tyul’bashev
机构
[1] Russian Academy of Sciences,Pushchino Radio Astronomy Observatory, Astro Space Center of the Lebedev Institute of Physics
来源
Astronomy Reports | 2001年 / 45卷
关键词
Magnetic Field; Physical Condition; Physical Parameter; Radio Source; Spectral Peak;
D O I
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中图分类号
学科分类号
摘要
Weak, compact radio sources (∼100 mJy peak flux, L∼1–10 pc) with their spectral peaks at about a gigahertz are studied, based on the complete sample of 46 radio sources of Snellen, drawn from high-sensitivity surveys, including the low-frequency Westerbork catalog. The physical parameters have been estimated for 14 sources: the magnetic field (H⊥), the number density of relativistic particles (ne), the energy of the magnetic field \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document} $$(E_{H_ \bot } )$$ \end{document}, and the energy of relativistic particles (Ee). Ten sources have \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document} $$E_{H_ \bot } \ll E_e $$ \end{document}, three have approximate equipartition of the energies \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document} $$(E_{H_ \bot } \sim E_e )$$ \end{document}, and only one has \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document} $$E_{H_ \bot } \gg E_e $$ \end{document}. The mean magnetic fields in quasars (10−3 G) and galaxies (10−2 G) have been estimated. The magnetic field appears to be related to the sizes of compact features as \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document} $$H \sim 1/\sqrt L $$ \end{document}.
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页码:428 / 433
页数:5
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