Volume 408, Number 3, September IV 2003
|Page(s)||961 - 969|
|Section||Interstellar and circumstellar matter|
|Published online||17 November 2003|
35 cm observations of a sample of large supernova remnants*
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
2 National Astronomical Observatories, CAS, Beijing 100012, China
Corresponding author: W. Reich, firstname.lastname@example.org
Accepted: 16 June 2003
We present radio maps of ten large-diameter supernova remnants observed at 35 cm wavelength with the Effelsberg 100-m telescope. The angular resolution is . The sources are G126.2+1.6, G127.1+0.5, HB3, HB9, S147, IC 443, Cygnus Loop, W63 and HB21. For each object we give an integrated flux density and improved spectra when necessary. We also present a map of G213.0-0.6, which we tentatively identify as a new large supernova remnant with a very low surface brightness, apparently interacting with the region S284.
Key words: ISM: supernova remnants / radio continuum: ISM
© ESO, 2003
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