Brightness and diameters for extragalactic SNRs (Urosevic+, 2005)

Details Brightness and diameters for extragalactic SNRs (Urosevic+, 2005) Brightness and diameters for extragalactic SNRs (Urosevic+, 2005)

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..34350437u&link_type=abstract

VizieR On-line Data Catalog: J/A+A/435/437. Originally published in: 2005A&A...435..437U

Physics

Galaxies: Radio, Galaxies: Nearby, Supernova Remnants

Scientific paper

This paper examines relations between the radio surface brightness Sigma and the diameter D (also known as Sigma-D relations) for a sample of extragalactic supernova remnants (SNRs) as constructed from a combination of published data and data from our own surveys. Our sample of extragalactic SNRs is the largest ever devised for the purpose of analyzing Sigma-D relations.
(1 data file).

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