Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...108..380z&link_type=abstract
Astronomy and Astrophysics, vol. 108, no. 2, Apr. 1982, p. 380-386.
Astronomy and Astrophysics
Astrophysics
4
Classifications, Computer Programs, Data Reduction, Digital Data, Stellar Spectra, A Stars, B Stars, Error Analysis, Galactic Structure, Line Spectra, Milky Way Galaxy, Minicomputers, Peculiar Stars, Stellar Evolution, Stellar Luminosity
Scientific paper
A method is presented to classify digitalized stellar spectra of normal stars of spectral classes B-K with respect to spectral class and absolute luminosity. The spectral class can be calculated with a mean error of 0.7 subclasses, but only the luminosities of B- and A-stars of classes V-III can be calculated with fair accuracy, while for the later spectral types more work with better standard spectra is necessary.
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