Rapid flux variations in compact radio sources

Details Rapid flux variations in compact radio sources Rapid flux variations in compact radio sources

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985acasn..26..197q&link_type=abstract

(Acta Astronomica Sinica, vol. 26, no. 3, 1985, p. 197-206) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 10, March

Astronomy and Astrophysics

Astrophysics

Extragalactic Radio Sources, Plasmons, Radiant Flux Density, Relativistic Velocity, Lorentz Force, Radiative Transfer, Variability

Scientific paper

The structure and flux variations noted in extragalactic radio sources may be related to the existence of relativistic bulk motion (or expansion) in the core region of compact radio sources. In the present consideration of the flux variation of a plasmon that is both moving and expanding relativistically, it is noted that large variations may result from even moderate values of the Lorentz factor for the expansion and the bulk motion. Attention is given to apparent shape in both polar and rectangular coordinates and to the solution of the equation of radiative transfer.

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