Interstellar scintillation and compact sources in supernova remnants

Details Interstellar scintillation and compact sources in supernova remnants Interstellar scintillation and compact sources in supernova remnants

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979natur.281...24c&link_type=abstract

Nature, vol. 281, Sept. 6, 1979, p. 24-27.

Other

9

Interstellar Extinction, Pulsars, Radio Scattering, Scintillation, Supernova Remnants, Brightness Temperature, Cross Correlation, Extragalactic Radio Sources, Spectral Correlation

Scientific paper

Interstellar scintillation was detected from a source in or near the supernova remnant G78.1 + 1.8, implying an angular size no greater than about 0.000001 arcsec, a brightness temperature above 10 to the 18th K, and a distance of about 3 kpc. The source does not seem to be a pulsar and is therefore the first source other than a pulsar to show interstellar scintillation. Limits are placed on the scintillating flux for 15 other galactic and extragalactic objects.

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