The Physics of Spectral Maxima in the Radiation from Non-Thermal Cosmic Radio Sources

Details The Physics of Spectral Maxima in the Radiation from Non-Thermal Cosmic Radio Sources The Physics of Spectral Maxima in the Radiation from Non-Thermal Cosmic Radio Sources

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap%26ss.302..189b&link_type=abstract

Astrophysics and Space Science, Volume 302, Issue 1-4, pp. 189-199

Astronomy and Astrophysics

Astrophysics

1

Radiation Mechanisms, Non-Thermal, Quasars, Radio Galaxies, Spectral Characteristic

Scientific paper

Universal expressions are presented for spectral characteristics of non-thermal cosmic radio sources which show maxima of the spectral density of radiation at specific frequencies (negative slopes spectra). For a number of quasars, radio galaxies and their individual details the most probable physical processes in space leading to spectra of the kind are determined, and some parameters of the space medium, magnetic field and angular sizes of compact radio sources are estimated.

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