Abstract
We report on new Australian Telescope Compact Array (ATCA) observations of SNR J0519-6902. The Supernova Remnant (SNR) is small in size (~8 pc) and exhibits a typical SNR spectrum of alpha = -0.53 ± 0.07, with steeper spectral indices found towards the northern limb of the remnant. SNR J0519-6902 contains a low level of radially orientated polarisation at wavelengths of 3 & 6 cm, which is characteristic of younger SNRs. A fairly strong magnetic field was estimated of ~171 microG. The remnant appears to be the result of a typical Type Ia supernovae, sharing many properties as another small and young Type Ia LMC SNR, J0509-6731.
Original language | English |
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Pages (from-to) | 25-33 |
Number of pages | 9 |
Journal | Serbian Astronomical Journal |
Volume | 185 |
DOIs | |
Publication status | Published - 2012 |
Keywords
- supernova remnants
- Magellanic Clouds
- radio continuum