Radio emission from very young supernova remnants - The case of SN 1979c

Details Radio emission from very young supernova remnants - The case of SN 1979c Radio emission from very young supernova remnants - The case of SN 1979c

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...245l.107p&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 245, May 1, 1981, p. L107, L108. Consiglio Nazionale delle Ricerche

Astronomy and Astrophysics

Astronomy

40

Radio Astronomy, Radio Sources (Astronomy), Supernova Remnants, Pulsars, Radio Emission

Scientific paper

The radio emission discovered from the one yr old remnant of the supernova in M100 (SN 1979c) is probably related to the energy output from a pulsar with a period P of about 10 ms. The lack of detectable emission at an earlier epoch may be due to synchrotron reabsorption, if P is about 1 ms. Some crucial observations are suggested. The case of SN 1970g may have been similar to the one under discussion.

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