On the surface brightness-diameter correlation for galactic supernova remnants

Details On the surface brightness-diameter correlation for galactic supernova remnants On the surface brightness-diameter correlation for galactic supernova remnants

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....54..915s&link_type=abstract

Astronomy and Astrophysics, vol. 54, no. 3, Feb. 1977, p. 915-918. Research supported by the Consiglio Nazionale delle Ricerche

Astronomy and Astrophysics

Astrophysics

13

Galactic Structure, Spectral Correlation, Stellar Luminosity, Supernova Remnants, Astrometry, Astronomical Catalogs, Brightness, Error Analysis

Scientific paper

Radio and optical observations of galactic supernova remnants (SNR) were compared in order to obtain information on the reliability of the surface brightness-diameter (Sigma-D) correlations proposed by different authors of SNR catalogs. Statistical diameters derived by Ilovaisky and Lequeux (1972) are found to be most reliable, while the catalogs of Milne (1970), Downes (1971), and Clark and Caswell (1976) present systematic errors in the statistical diameter determination

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