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

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

2008-04-29

arxiv.org/abs/0804.4537v1

Astronomy and Astrophysics

Astrophysics

6 pages 4 figures, to be published in Serbian Astronomical Journal

Scientific paper

10.2298/SAJ0876059C

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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