Chemical abundances in the globular clusters NGC6229 and NGC6779 [Fe/H] as well as the first estimate of the abundances of C,
N, O, Mg, Ca, Ti, and Cr
Age and chemical composition of the globular cluster NGC 6652 of determination of the age, helium mass fraction (Y), metallicity ([Fe/H]), and abundances of the elements C,
N, O
Age, Helium Content and Chemical Composition of Globular Clusters in the M31 Neighborhood and in our Galaxy (Y), metallicity ([Fe/H]), and estimations of abundances of the elements: C,
N, O, Mg, Ca, Ti, Cr, Ni
Gemini spectroscopy of the outer disk star cluster BH176 objects. Results. We determine the following parameters for BH176: Vh = 0 ± 15 km
s-1, [Fe/H] = -0.1 ± 0
Chemical abundances in the globular clusters NGC6229 and NGC6779 [Fe/H] as well as the first estimate of the abundances of C,
N, O, Mg, Ca, Ti, and Cr