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

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

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008arep...52..201m&link_type=abstract

Astronomy Reports, Volume 52, Issue 3, pp.201-210

Astronomy and Astrophysics

Astronomy

98.70.Dk, 98.62.En, 98.62.Lv, 95.30.Gv, Radio Sources, Radio Sources, Electric And Magnetic Fields, Stellar Content And Populations, Radii, Morphology And Overall Structure, Radiation Mechanisms, Polarization

Scientific paper

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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