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Radio observations of the extended supernova remnants (SNRs) N23 : SNR, N120 : SNR, 0525[660, N49, and N44 : shell 3 in the Large Magellanic Cloud show a variety of structures and little di †erence from shell SNRs in the Milky Way. N23 : SNR and N120 : SNR have very regular outlines, but the shells are much brighter on the sides toward the most prominent parts of their associated H II region complexes, probably reÑecting density gradients in the surroundings. N23 : SNR has a mixed magnetic Ðelddoi:10.1086/300246 fatcat:wcvbjpue7zenzhl5vmxpwp5jia