Radio-continuum study of MCSNR J0536-7038 (DEM L249)

preprint2014arXivOpen access

Abstract

We present a detailed radio-continuum study on Australia Telescope Compact Array (ATCA) observations of Large Magellanic Cloud (LMC) supernova remnant (SNR), MCSNR 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 α=−0.52±0.07α=-0.52\pm0.07 between λ=73λ= 73 and 6 cm. We report detections of regions showing moderately high fractional polarisation at 6 cm, with a peak value of 71±\pm25% and a mean fractional polarisation of 35±\pm8%. We also estimate an average rotation measure across the remnant of -237 rad m−2^{-2}. The intrinsic magnetic field appears to be uniformly distributed, extending in the direction of the two brightened limbs of the remnant.

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