Ghavam et al. present new ATCA radio observations toward N49, one of the brightest supernova remnants (SNRs) located in the Large Magellanic Cloud (LMC). New and archival ATCA radio observations were analysed along with Chandra X-ray data. These observations confirm a prominent “bullet” shaped feature beyond the southwestern boundary of the SNR. Both X-ray morphology and radio polarisation analysis support a physical connection of this feature to the SNR. The “bullet’s” apparent velocity is estimated to be ∼1300 km/s, based on its distance (∼10 pc) from the remnant’s geometric centre and estimated age (∼7600 yrs). The radio spectral index is estimated to be –0.55 which is typical of middle-age supernova remnants (SNRs). The image above is an X-ray three-colour image of N49 that shows the new ATCA data superimposed as contours. Red represents the energy band 0.5–1.2 keV (soft), green corresponds to the energy band 1.2–2.0 keV (Medium) and blue represents the energy band 2.0–7.0 keV (hard). This X-ray image is overlaid with 5.5 GHz radio contours at 0.25, 1.4, 2.6, 3.8, and 5 mJy/beam. The location of the “bullet”, a presumed knot of ejecta from the SNR, is shown.