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Author

S. Lazarević

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Open access Oct 2026

Radio Continuum Study of One of the Brightest Large Magellanic Cloud Supernova Remnants N 132D

We present a new radio continuum study of the Large Magellanic Cloud supernova remnant N 132D using observations from the Australia Telescope Compact Array (ATCA) and MeerKAT. The radio morphology shows a clear spatial correlation with the X-ray emission in the central and left regions of the remnant, as well as in the...

R. Alsaberi, Z. Smeaton, M. Filipović et al. · 0 citations

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