High-resolution radio observations of three supernova remnants

Details High-resolution radio observations of three supernova remnants High-resolution radio observations of three supernova remnants

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...204..427b&link_type=abstract

Astrophysical Journal, vol. 204, Mar. 1, 1976, pt. 1, p. 427-440.

Astronomy and Astrophysics

Astronomy

30

Astronomical Spectroscopy, Brightness Temperature, Radio Astronomy, Supernova Remnants, Emission Spectra, High Resolution, Line Spectra, Parabolic Antennas, Radiant Flux Density, Spectral Bands, Telescopes

Scientific paper

The paper presents and discusses radio observations of three supernova remnants (G21.5-0.9, G29.7-0.3, and 3C 391) made at 3.7 and 11.1 centimeters. The supernova remnant G21.5-0.9 has an elliptical brightness distribution and is similar to the Crab Nebula as well as 3C 58 in appearance and spectrum. The two remnants G29.7-0.3 and 3C 391 both show a broken shell structure typical of most galactic supernova remnants.

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