Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Astronomical Observatory of Odessa National University
GEPI
Department of Astronomy and Astronomical Observatory, Odessa National University
INAF-Osservatorio Astronomico di Palermo
Department of Astronomy and Astronomical Observatory, Odessa, Ukraine
Department of Astronomy and Astronomical Observatory, Odessa National University, T.G. Shevchenko Park, 65014 Odessa, Ukraine; Isaac Newton Institute of Chile, Odessa Branch, Ukraine
Department of Astronomy, Odessa State University, Shevchenko Park, 65014 Odessa, Ukraine ; Odessa Astronomical Observatory and Isaac Newton Institute of Chile, Odessa Branch, Ukraine
Astronomical Observatory, Mechnikov National University
Department of Astronomy, Odessa State University, Shevchenko Park, 270014 Odessa, Ukraine of Astronomy, Odessa State University, Shevchenko Park, 270014, Odessa, Ukraine of Astronomy, Odessa State University, Shevchenko Park, 65014, Odessa, Ukraine
Department of Astronomy, Odessa State University, Shevchenko Park, 270014 Odessa, Ukraine Observatoriia, Odessa, Ukrainian SSR
Department of Astronomy, Odessa State University, Shevchenko Park, 65014 Odessa, Ukraine; Isaac Newton Institute in Chile, Odessa Branch
Department of Astronomy and Astronomical Observatory, Odessa National University, T.G. Shevchenko Park, 65014 Odessa, Ukraine, and Isaac Newton Institute of Chile, Odessa Branch, Ukraine
Astronomical Observatory, Odessa National University T.G. Shevchenko Park, Odessa 65014, Ukraine
Department of Astronomy, Odessa State University, Shevchenko Park, 65014, Odessa, Ukraine; Isaac Newton Institute of Chile, Odessa Branch
Department of Astronomy, Odessa State University, Shevchenko Park, 65014 Odessa, Ukraine; Isaac Newton Institute of Chile, Odessa Branch, Ukraine
Astronomical Obse
Abundances of giants in four Galactic clusters (Sestito+, 2008)
Abundances of stars in lower main sequence (Mishenina+, 2008)
An influence of the cool star chromospheres on the 4571 A magnesium line
Barium abundance in red giants of NGC 6752. Non-local thermodynamic equilibrium and three-dimensional effects
Carbon and nitrogen abundances in early B-stars. I. NLTE calculations for a sample of stars with small V sin i values
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Profile ID: LFWR-SCP-P-121902