Radio observations of a new galactic supernova remnant, G9.8 + 0.6

Details Radio observations of a new galactic supernova remnant, G9.8 + 0.6 Radio observations of a new galactic supernova remnant, G9.8 + 0.6

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.204..833c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 204, Aug. 1983, p. 833-836.

Astronomy and Astrophysics

Astronomy

11

Milky Way Galaxy, Radio Sources (Astronomy), Supernova Remnants, Astronomical Maps

Scientific paper

A new map at 408 MHz made with the Molonglo Cross shows that the radio source G9.8+0.6 has a broken shell structure and a non-thermal spectral index. These facts, together with the proximity of the source to the galactic equator, indicate that it is a previously unrecognized galactic supernova remnant. The remnant is an example of a shell which is much brighter on the side towards the galactic plane. The author estimates its distance, size and age from its measured radio parameters.

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