Evolution of the radio emission from young SNRs according to observational data

Details Evolution of the radio emission from young SNRs according to observational data Evolution of the radio emission from young SNRs according to observational data

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aujph..32...95s&link_type=abstract

(Joint Australia-USSR-USA Symposium on Pulsars and Supernova Remnants, Sydney, Australia, Apr. 1978.) Australian Journal of Phys

Physics

7

Radiant Flux Density, Radio Emission, Radio Spectra, Supernova Remnants, Radio Bursts, Secular Variations, Spectral Energy Distribution, Stellar Radiation

Scientific paper

Results are given from a still-continuing series of absolute flux density measurements for the SNR Cas A. The measurements have been taken regularly over the past 16 years at 24 wavelengths in the range 3-60 cm. New data are presented for the rate of flux density decrease, and for time and frequency variations in the spectral index. Intensity increases that are localized in frequency are described. The results are generalized in a model for the radio emission from a young SNR, and this is used to analyze experimental data for flux density decreases in the emission from 3C 10 and 58.

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