Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980azh....57...53m&link_type=abstract
Astronomicheskii Zhurnal, vol. 57, no. 1, 1980, p. 53-64. In Russian.
Astronomy and Astrophysics
Astronomy
4
Chemical Composition, Galactic Evolution, Galactic Structure, Main Sequence Stars, Milky Way Galaxy, Stellar Structure, Abundance, Astronomical Photometry, Chemical Evolution, Dwarf Stars, F Stars, G Stars, K Stars, Kinematics, Star Distribution, Ubv Spectra, Ultraviolet Radiation
Scientific paper
Metallicity indices deltaO.6, DeltaR-1(U-B), and delta(m1)(beta) have been calculated for eight samples of main-sequence disk stars. Indices deltaO.6 and Delta(U-B) have been calibrated to the metal abundance (Fe/H) for the spectral types F, G, and K separately. It is shown that the actual metal abundance distribution among the disk stars is essentially discrete. The UBV and RI data for the F- and K-dwarfs imply that the metallicity of the sun coincides with that of the Hyades, whereas the G-dwarf data yield the known smaller metallicity of the sun with respect to the Hyades. The results are discussed with reference to the chemical evolution of the Galaxy.
Marsakov V. A.
Suchkov Anatoly A.
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