We present a detailed radio-continuum study on Australia Telescope Compact Array ( ATCA ) observations of Large Magellanic Cloud ( LMC ) supernova remnant ( SNR ) , MCSNRÂ J0536–7038 .
This Type Ia SNR follows a horseshoe morphology , with a size 32 pc \times 32 pc ( 1-pc uncertainty in each direction ) .
It exhibits a radio spectrum \alpha = -0.52 \pm 0.07 between \lambda = 73 and 6Â cm .
We report detections of regions showing moderately high fractional polarisation at 6Â cm , with a peak value of 71 \pm 25 % and a mean fractional polarisation of 35 \pm 8 % .
We also estimate an average rotation measure across the remnant of –237 rad m ^ { -2 } .
The intrinsic magnetic field appears to be uniformly distributed , extending in the direction of the two brightened limbs of the remnant .