This webpage presents images and accompanying radio synchrotron emission models of all known Supernova Remnants (SNRs) in the Galaxy (excluding pulsar wind nebulae, also known as "filled-centre" SNRs). The underlying database uses the University of Manitoba's High-Energy Catalogue of Supernova Remnants (SNRcat) (companion paper: A census of high-energy observations of Galactic supernova remnants by Ferrand, G., Safi-Harb, S., 2012, AdSpR, 49, 9, 1313-1319. ADS link).
This webpage is a supplement to the paper: The Connection between Supernova Remnants and the Galactic Magnetic Field: I. A Global Radio Study of the Axisymmetric Sample (West, J. L., Safi-Harb, S., Jaffe, T., Kothes, R., Foster, T., & Landecker, T., 2016, A&A, 587, 148).
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