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 |
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Hauptverfasser: | , , , |
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] |
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ISSN: | 0571-7256 1573-8191 |
DOI: | 10.1023/A:1020199802755 |