Spectrum of the variable component of the radio source J0157+7442

Details Spectrum of the variable component of the radio source J0157+7442 Spectrum of the variable component of the radio source J0157+7442

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010arep...54..983g&link_type=abstract

Astronomy Reports, Volume 54, Issue 11, pp.983-985

Astronomy and Astrophysics

Astronomy

Scientific paper

The spectrum of the maximum values of the variable component of the radio source J0157+7442 is presented. The flux densities obtained on the RATAN-600 radio telescope at centimeter wavelengths in 2009 and 2010 are minimum for all observations of the source, and it was assumed that the variable component was absent in these years. After subtracting these RATAN-600 data from the upper envelope of all available flux density data, the spectrum of the variable component was obtained. The form of the spectrum of the variable component is typical of a nonuniform, spherically symmetric source with synchrotron self-absorption.

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