Radio Continuum Study of Supernova Remnants in the Large Magellanic Cloud - SNR J0519-6926


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We present the results of new high resolution ATCA observations of SNR J0519-6926. We found that this SNR exhibits a typical horseshoe appearance with alpha = -0.55 +- 0.08 and D=28+-1 pc. No polarization (or magnetic fields) are detected to a level of 1%. This is probably due to a relatively poor sampling of the uv plane caused be observing in snap-shot mode.

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