
%0 Journal Article
%A Kesteven, MJ 
%A Caswell, JL 
%A Roger, RS 
%A Milne, DK 
%A Haynes, RF 
%A Wellington, KJ 
%T Supernova Remnants with Jets
%J Australian Journal of Physics
%D 1987/12/01
%V 40
%N 6
%P 855-860
%K 
%R https://doi.org/10.1071/PH870855
%U https://www.publish.csiro.au/paper/PH870855 
%X Two examples are given of probable radio jet/supernova remnant associations: G332.4+0·1 and G 315 ·8 - O· O. In both cases the jet length is larger than the radius of the remnant's shell, and the jet diameter is barely resolved and substantially less than the observed shell thickness. The jet luminosity is 5-10% that of the shell. The G332·4 +0.1 jet terminates 'in an extended plume whose luminosity is about 50% that of the shell. 
