ON THE TIME FREQUENCY DEPENDENCIES OF THE SECULAR DECREASE RATE OF CASSIOPEIA A RADIO EMISSION
Flux densities of young supernova remnant Cassiopeia A relative to those for radiogalaxy Cygnus A were measured in 1977-1992 at the frequencies of 290 and 927 MHz. These measurements were made with the same 10 m radiotelescopes at the Staraya Pustyn Radioastronomical Observatory (NIRFI). Decline of...
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| Format: | Article |
| Language: | English |
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Odessa I. I. Mechnykov National University
2017-07-01
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| Series: | Odessa Astronomical Publications |
| Online Access: | http://oap.onu.edu.ua/article/view/105799 |