Variation of Flux Density of the Radio Source Cassiopeia A

Details Variation of Flux Density of the Radio Source Cassiopeia A Variation of Flux Density of the Radio Source Cassiopeia A

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ap.....45..365m&link_type=abstract

Astrophysics (English translation of Astrofizika), v. 45, Issue 3, p. 365-369 (2002).

Astronomy and Astrophysics

Astrophysics

1

Stars - Stars Supernovae - Radio Continuum Stars - Individual Cassiopeia A

Scientific paper

The character of the yearly average and secular variations of the intensity of the radio emission of Cassiopeia A is discussed on the basis of multiyear observations (1953-2001) made at Byurakan Astrophysical Observatory and the Institute of Radiophysics and Electronics. It is shown that in this period the intensity of the radio emission of Cassiopeia A has decreased by about 34%, at a yearly average rate of 0.7%.

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