Radio-Continuum Study of the Supernova Remnants in the Large Magellanic Cloud - An SNR with a Highly Polarised Breakout Region - SNR J0455-6838

Details Radio-Continuum Study of the Supernova Remnants in the Large Magellanic Cloud - An SNR with a Highly Polarised Breakout Region - SNR J0455-6838 Radio-Continuum Study of the Supernova Remnants in the Large Magellanic Cloud - An SNR with a Highly Polarised Breakout Region - SNR J0455-6838

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008seraj.177...61c&link_type=abstract

Serbian Astronomical Journal, vol. 177, pp. 61-66

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6

Ism: Supernova Remnants, Magellanic Clouds, Radio Continuum: Ism, Polarization, Ism: Individual Objects: Snr J0455-6838

Scientific paper

We present the results of new moderate resolution ATCA observations of SNR J0455-6838. We found that this SNR exhibits a mostly typical appearance with rather steep and curved α=--0.81±0.18 and D=43×31±1~pc. Regions of high polarisation were detected, including unusually strong (˜70%) region corresponding to the northern breakout. Such a strong polarisation in breakout regions has not been observed in any other SNR.

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