Radio observations of the supernova remnant G 109.1-1.0

Details Radio observations of the supernova remnant G 109.1-1.0 Radio observations of the supernova remnant G 109.1-1.0

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.203..695d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 203, May 1983, p. 695-699.

Astronomy and Astrophysics

Astronomy

15

Radio Astronomy, Supernova Remnants, X Ray Sources, Astronomical Maps, Pulsars

Scientific paper

The supernova remnant G 109.1-1.0, which contains a periodic X-ray point source, has been observed with the Effelsberg 100-m telescope at 2.7 GHz. The remnant has shell structure at both radio and X-ray wavelengths and the radio and X-ray maps show similar large-scale emission. No linearly polarized radio emission was detected. G 109.1-1.0 is one of three shell remnants in which the probable stellar remnant has now been found.

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