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T.G. Pannuti, N. Duric (UNM)
Using X-ray, optical and radio observations, we have conducted a multi-wavelength search for supernova remnants in three Sculptor Group galaxies (NGC 247, NGC 300 and NGC 7793). Characteristics and multi-wavelength properties of the detected remnants will be presented and discussed.
The author(s) of this abstract have provided an email address for comments about the abstract: tpannuti@astro.phys.unm.edu