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

Abstract

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.

arXiv comment6 pages 4 figures, to be published in Serbian Astronomical Journal

References in corpus (2)

• An ATCA 20cm Radio Continuum Study of the Large Magellanic Cloud
• Multi-frequency Study of the LMC Supernova Remnant (SNR) B0513-692 and New SNR Candidate J051327-6911

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• ALMA CO Observations of Supernova Remnant N63A in the Large Magellanic Cloud: Discovery of Dense Molecular Clouds Embedded within Shock-Ionized and Photoionized Nebulae
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• Multi-frequency observations of a superbubble in the LMC: The case of LHA 120-N 70
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