35 cm observations of a sample of large supernova remnants

Details 35 cm observations of a sample of large supernova remnants 35 cm observations of a sample of large supernova remnants

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003a%26a...408..961r&link_type=abstract

Astronomy and Astrophysics, v.408, p.961-969 (2003)

Astronomy and Astrophysics

Astrophysics

21

Ism: Supernova Remnants, Radio Continuum: Ism

Scientific paper

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 14farcm5 . 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 H Ii region S284.
Based on observations with the Effelsberg 100-m telescope operated by the Max-Planck-Institut für Radioastronomie (MPIfR), Bonn, Germany.

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