Variation of Flux Density of the Radio Source Cassiopeia A

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...

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Veröffentlicht in:Astrophysics 2002-07, Vol.45 (3), p.365-369
Hauptverfasser: Martirossyan, R M, Goulyan, A G, Sanamyan, V A, Manaselyan, Kh A
Format: Artikel
Sprache:eng
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Zusammenfassung: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%.[PUBLICATION ABSTRACT]
ISSN:0571-7256
1573-8191
DOI:10.1023/A:1020199802755