Radio emission in active galaxies - The starburst scenario

Details Radio emission in active galaxies - The starburst scenario Radio emission in active galaxies - The starburst scenario

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.205...99c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 205, no. 1, p. 99-105.

Astronomy and Astrophysics

Astronomy

Active Galaxies, Nuclear Radiation, Radio Emission, Starburst Galaxies, Infrared Astronomy Satellite, Supernova Remnants

Scientific paper

The origin of the radio emission in active galaxies ranging from LINERS to ultraluminous IRAS galaxies is considered under the scenario of a violent nuclear or circumnuclear starburst. The radio luminosity is explained as non-thermal radio emission generated in supernova remnants (SNRs). Implications of this scenario in terms of the radio brightness of SNRs, the supernovae rates, and their detectability are discussed.

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