G279.0 + 1.1 - A new large-diameter galactic supernova remnant

Details G279.0 + 1.1 - A new large-diameter galactic supernova remnant G279.0 + 1.1 - A new large-diameter galactic supernova remnant

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.234..971w&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 234, Oct. 15, 1988, p. 971-975. Research supported by R

Astronomy and Astrophysics

Astronomy

8

Brightness, Radio Sources (Astronomy), Supernova Remnants, Carbon Monoxide, Data Reduction, H I Regions, Milky Way Galaxy

Scientific paper

The authors present radio continuum maps at 2325 and 1644 MHz of a new large-diameter supernova remnant (SNR) centred on l = 279°.0, b = +1°.1. The angular diameter of the SNR shell is 1°.6, and the estimated linear diameter is 84 pc. These new observations are compared with other radio and optical data. It would appear that no optical emission has been detected which is associated with the radio source.

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