32 GHz radio continuum observations of four shell-type supernova remnants

Details 32 GHz radio continuum observations of four shell-type supernova remnants 32 GHz radio continuum observations of four shell-type supernova remnants

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...71..189m&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 71, no. 2, Nov. 1987, p. 189-195.

Astronomy and Astrophysics

Astronomy

18

Astronomical Maps, Millimeter Waves, Noise Temperature, Radio Astronomy, Radio Spectra, Supernova Remnants, Continuous Spectra, High Resolution, Radiant Flux Density

Scientific paper

A series of 32-GHz maps obtained with the Effelsberg 100-m telescope of
the four supernova remnants G11.2-0.3, G29.7-0.3, G41.1-0.3 and
G43.3-0.2 is presented. The radio spectra of these sources are
discussed. G11.2-0.3 seems to belong to the class of supernova remnants
showing both shell-type and plerionic characteristics.

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