Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..348k&link_type=abstract
(Astronomicheskii Zhurnal, vol. 62, Mar.-Apr. 1985, p. 348-355) Soviet Astronomy (ISSN 0038-5301), vol. 29, Mar.-Apr. 1985, p. 2
Astronomy and Astrophysics
Astronomy
1
Colorimetry, Stellar Composition, Stellar Luminosity, Ubv Spectra, Astronomical Catalogs, Cosmic Dust, Heavy Elements, Star Distribution, Stellar Color
Scientific paper
A true-color line, i.e., a (U-B)0, (U-B)0(K) diagram, is constructed for O5-K5 stars of luminosity class V with the solar chemical composition (Fe/H = 0). Through a comparison with the corresponding diagram for stars of luminosity class V obtained by Straizys, it is established that for O5 V-K3 stars the difference in color indices is /Delta (B-V)0/ = /(B-V)0(K) - (B-V)0(1)/ less than 0.003 m, i.e., the two (B-V)0 systems practically coincide.
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