
%0 Journal Article
%A Dickel, JR 
%A Milne, DK 
%A Kerr, AR 
%A Ables, JG 
%T 8·8 GHz Radio Observations of 12 Suggested Supernova Remnants
%J Australian Journal of Physics
%D 1973/06/01
%V 26
%N 3
%P 379-388
%K 
%R https://doi.org/10.1071/PH730379
%U https://www.publish.csiro.au/paper/PH730379 
%X Brightness distributions and flux densities at 8·8 GHz are presented for 12 small-diameter radio sources near the galactic plane. Each of these sources has been classified at one time or another as a supernova remnant. For one source, G295· 2 - 0·6, the flux density at 8·8 GHz confirms the thermal spectrum suggested by lower frequency measurements and indicates that it is not a supernova remnant. Another source, G309· 6+ 1·7, is thought to be extragalactic. 
