An X-ray, Optical and Radio Search for Supernova Remnants in the Sculptor Group Galaxies NGC 247, NGC 300 and NGC 7793

Details An X-ray, Optical and Radio Search for Supernova Remnants in the Sculptor Group Galaxies NGC 247, NGC 300 and NGC 7793 An X-ray, Optical and Radio Search for Supernova Remnants in the Sculptor Group Galaxies NGC 247, NGC 300 and NGC 7793

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...195.3307p&link_type=abstract

American Astronomical Society, 195th AAS Meeting, #33.07; Bulletin of the American Astronomical Society, Vol. 31, p.1418

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Scientific paper

The study of supernova remnants (SNRs) in nearby galaxies offers the opportunity to examine the properties of an entire sample of sources without the limitations typically encountered in the study of Galactic SNRs. Using observations made at the X-ray, optical and radio wavelengths of the Sculptor Group galaxies NGC 247, NGC 300 and NGC 7793, we have examined the positions of previously-known optically-identified SNRs for emission at the other two wavelengths, as well as searched for new candidate X-ray and radio SNRs. Initial results and tentative conclusions will be presented.

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