G309.2โ00.6 and jets in supernova remnants
G309.2โ00.6 and jets in supernova remnants
We present Australia Telescope Compact Array observations of the supernova remnant (SNR) G309.2โ00.6. In a 1.3-GHz continuum image the remnant appears as a near-circular shell, but with two brightened and distorted arcs of emission on opposite sides. H i absorption against the SNR yields a distance in the range 5.4 โฆ