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Secular decrease in the 927-MHz flux of the supernova remnants Cassiopeia A and Taurus A

Journal Article · · Sov. Astron. AJ (Engl. Transl.); (United States)
OSTI ID:5556312
Relative measurements of the radio flux density of the supernova remnants Cas A and Tau A at 927-MHz frequency were carried out with the 10-m radio telescope of the Staraya Pustyn' station, Gor'kii Radiophysics Institute, in October--December 1977. The Orion Nebula and the radio galaxies Cygnus A and Virgo A served as comparison sources. Comparison of the results with absolute measurements made in October 1962 indicates that over the 15-yr interval the radio flux of Cas A dropped by (14.2 +- 0.6) % (mean annual decrease, (0.95 +- 0.04) %), while the Tau A flux dropped by (2.7 +- 0.1) % (mean annual decrease, (0.18 +- 0.01) %).
Research Organization:
Gor'kii Radiophysics Institute
OSTI ID:
5556312
Journal Information:
Sov. Astron. AJ (Engl. Transl.); (United States), Journal Name: Sov. Astron. AJ (Engl. Transl.); (United States) Vol. 23:5; ISSN SAAJA
Country of Publication:
United States
Language:
English

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