Radio lines observations in the direction of several supernova remnants

Details Radio lines observations in the direction of several supernova remnants Radio lines observations in the direction of several supernova remnants

Jul 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....50..259c&link_type=abstract

Astronomy and Astrophysics, vol. 50, no. 2, July 1976, p. 259-262.

Astronomy and Astrophysics

Astronomy

2

Interstellar Matter, Radio Astronomy, Supernova Remnants, Carbon Stars, H Ii Regions, Line Spectra, Microwave Emission, Recombination Reactions

Scientific paper

The present observations were performed to investigate a possible correlation between the free-free absorption and the recombination line emission. None was found, possibly due to the lack of angular resolution. We did find however, a number of carbon recombination line sources. Carbon emission had been previously detected generally in the direction of H II regions and more recently in a few dark clouds.

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