Model integrated B - V colors for metal-poor stellar systems

Details Model integrated B - V colors for metal-poor stellar systems Model integrated B - V colors for metal-poor stellar systems

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..501s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, July 1984, p. 501-507) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, July-Aug

Astronomy and Astrophysics

Astronomy

Colorimetry, Globular Clusters, Stellar Color, Stellar Models, Stellar Systems, Abundance, Chronology, Metallicity

Scientific paper

The B-V colour is calculated for stellar systems without star formation having metallicities Z = 10-3 and 10-4 and ages T = 7 and 18 billion years. Results of model calculations are consistent with the new metallicity scale of globular clusters. The ages of relatively metal-rich globular clusters ([Fe/H] > -1.2) and M92 are roughly estimated.

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