An automated determination of the absolute magnitudes of stars in the Vilnius photometric system

Details An automated determination of the absolute magnitudes of stars in the Vilnius photometric system An automated determination of the absolute magnitudes of stars in the Vilnius photometric system

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26as...95..417s&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 95, no. 3, p. 417-422.

Astronomy and Astrophysics

Astrophysics

2

Astrometry, Astronomical Photometry, Stellar Magnitude, Astronomical Catalogs, Stellar Luminosity

Scientific paper

The possibility of extending the previously automated comparison method of Smriglio et al. (1986) for the determination of the absolute magnitudes of stars, M(V), was investigated by applying the same criterion which was used in Smriglio et al. method in the determination of spectal types and luminosity classes (i.e., by using the Vilnius seven-color photometric system). Absolute magnitudes of stars obtained by this method were found to agree well with the M(V) values obtained using other methods, including the uses of calibrated Q-Q diagrams, the MK type-M(V) map by Straizys and Kuriliene (1981), and the MK type-M(V) map by Corbally and Garrison (1984).

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