The nature of bilateral supernova remnants

We present high-resolution radio images at 1.4 GHz of two Galactic supernova remnants (SNRs), G003.8–00.3 (formerly G003.7–00.2) and G350.0– 02.0 (formerly G350.0-01.8). Although the two objects are very different in appearance, in both cases the radio emission shows a clear bilateral (or “barrel”) morphology for which the axis is parallel to the Galactic Plane. The majority of Galactic SNRs have now been observed at high resolution, and one can define a clear bilateral subset of the population. We consider a sample of 17 such SNRs, and find a highly significant tendency for the bilateral axes of these SNRs to be aligned with the Galactic Plane. We interpret this as indicating that “extrinsic” effects dominate the morphology of such remnants. Specifically, we argue that the Galactic magnetic field causes these SNRs to appear bilateral, either directly, in the form of magnetic field compression and/or quasi-perpendicular acceleration of electrons in the supernova shock, or more likely indirectly, by pre-processing the interstellar medium to produce density stratifications extended along the Plane. Subject headings: Galaxy: structure — ISM: magnetic fields, structure — shock waves — supernova remnants: individual (G003.8–00.3, G350.0–02.0) Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 2121, Australia Astrophysics Department, School of Physics A29, University of Sydney, NSW 2006, Australia; [email protected]