The radio emission of galaxies and their supernova rate

Details The radio emission of galaxies and their supernova rate The radio emission of galaxies and their supernova rate

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61..234s&link_type=abstract

(Astronomicheskii Zhurnal, vol. 61, Mar.-Apr. 1984, p. 234-239) Soviet Astronomy (ISSN 0038-5301), vol. 28, Mar.-Apr. 1984, p. 1

Astronomy and Astrophysics

Astronomy

2

Galactic Radio Waves, Radio Emission, Supernova Remnants, Luminosity, Nonthermal Radiation, Pulsars, Radio Spectra, Stellar Models

Scientific paper

Taking into account the radial distribution of SNRs, the rate of galactic supernovae is determined. On the basis of an empirical model of SNR evolution the contribution of the remnants to the radio emission of galaxies has been quantitatively estimated and the rate of supernovae in some of the galaxies has been calculated. A correlation between the supernovae rate and the power of the non-thermal radio emission of spiral and irregular galaxies is established.

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