5 GHz observations of galactic supernova remnants

Details 5 GHz observations of galactic supernova remnants 5 GHz observations of galactic supernova remnants

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....55...11a&link_type=abstract

Astronomy and Astrophysics, vol. 55, no. 1, Feb. 1977, p. 11-18.

Astronomy and Astrophysics

Astronomy

23

Galactic Radiation, Microwave Emission, Radio Sources (Astronomy), Supernova Remnants, Thermal Emission, Astronomical Maps, Brightness, Luminous Intensity, Polarization Characteristics

Scientific paper

Brightness and polarization distributions over several galactic supernova remnants have been observed at a wavelength of 6 cm. These observations have confirmed the nonthermal nature of most of the observed sources. It is suggested, however, that the objects G33.1-0.1 (KES 78), G35.6-0.0, G37.6-0.1, G37.7+0.1, and G37.9-0.4 are thermal. The results of these observations are presented in the form of total intensity contour maps with superimposed polarization vectors.

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