Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981azh....58..516t&link_type=abstract
Astronomicheskii Zhurnal, vol. 58, May-June 1981, p. 516-523. In Russian.
Astronomy and Astrophysics
Astrophysics
Brightness Temperature, Electromagnetic Absorption, Extragalactic Radio Sources, Relativistic Electron Beams, Synchrotron Radiation, Compton Effect, Electron Energy, Energy Spectra, Quasars, Very Long Base Interferometry
Scientific paper
It is shown that electrons in sources with high brightness temperatures of cyclotron radiation can, in the average, acquire energy through reabsorption despite catastrophic Compton losses. The brightness temperature of stationary sources with synchrotron reabsorption depends only on the energies of the radiating electrons, and if these energies exceed 200 mc-squared, then the brightness temperature can exceed 10 to the 12th K. Consideration is given to the formation of stationary distributions in sources with synchrotron reabsorption, and an analysis is presented of possible limits on the brightness temperature of synchrotron radiation in stationary sources (i.e., synchrotron reactors). Two examples, the quasar 3C 273 and Cen A, are considered
Charugin V. M.
Tsvetanov Zlatan I.
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