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We present a study of new Australian Telescope Compact Array (ATCA)observations of supernova remnant, SNR J0536-6735. This remnant appears tofollow a shell morphology with a diameter of D=36x29 pc (with 1 pc uncertaintyin each direction). There is an embedded Hii region on the northern limb of theremnant which made various analysis and measurements (such as flux density,spectral index and polarisation) difficult. The radio-continuum emissionfollowed the same structure as the optical emission, allowing for extent andflux density estimates at 20 cm. We estimate a surface brightness for the SNRat 1 GHz of 2.55x10^-21 W m^-2 Hz^-1 sr^-1. Also, we detect a distinctiveradio-continuum point source which confirms the previous suggestion of thisremnant being associated with a pulsar wind nebulae (PWN). The tail of thisremnant isn't seen in the radio-continuum images and is only seen in theoptical and X-ray images.

Multifrequency radio observations of SNR J0536-6735 (N 59B) with associated pulsar