Radio continuum observations of the supernova remnants G 127.1 + 0.5 and G 126.2 + 1.6 at 11 CM and 6 CM wavelength

Astronomy and Astrophysics – Astronomy

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Astronomical Maps, Centimeter Waves, Linear Polarization, Microwave Spectra, Radio Astronomy, Supernova Remnants, Angular Resolution, Astronomical Spectroscopy, Interstellar Matter, Radiant Flux Density, Radio Observation, Radio Telescopes

Scientific paper

Radio observations with the Effelsberg 100 m telescope of the two supernova remnants G 127.1 + 0.5 and G 126.2 + 1.6, at 11 cm and 6 cm wavelength, are presented. In the case of G 127.1 + 0.5, linear polarization data were obtained and used for the investigation of the magnetic field distribution. All radio data were found to be consistent with the van der Laan (1962) model. G 126.2 + 1.6 has been observed only in total power; a spectral steepening beyond about 3 GHz is indicated.

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