32 GHz radio continuum observations of four plerionic supernova remnants

Details 32 GHz radio continuum observations of four plerionic supernova remnants 32 GHz radio continuum observations of four plerionic supernova remnants

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...69..533m&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 69, no. 3, June 1987, p. 533-540.

Astronomy and Astrophysics

Astrophysics

30

Astronomical Maps, Continuous Spectra, Radio Spectra, Stellar Spectrophotometry, Supernova Remnants, Millimeter Waves, Spectral Energy Distribution, Stellar Models

Scientific paper

Maps made at 32 GHz with the Effelsberg 100-m telescope of the source Tau A, G 21.5-0.9, 3C 58 and G 74.9+1.2 are presented. The spectra of Tau A, G 21.5-0.9 and 3C 58 show no deviation from their low-frequency extrapolation. G 74.9+1.2 shows a spectral break above 11 GHz. The consequences for models of plerionic supernova remnants are briefly discussed.

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