Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
GEPI
Odessa State University, Ukraine
INAF-Osservatorio Astronomico di Palermo
Department of Astronomy and Astronomical Observatory, Odessa National University
GEPI, UMR CNRS, Observatoire de Paris, France
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany, ; and Odessa State University, Department of Astronomy, Shevchenko Park, 270014 Odessa, Ukraine State University, Odessa, Ukraine
GEPI, Observatoire de Paris-Meudon, 92125 Meudon Cedex, France; Department of Astronomy and Astronomical Observatory, Odessa National University, T.G. Shevchenko Park, 65014 Odessa, Ukraine; Isaac Newton Institute of Chile, Odessa Branch, Ukraine of Astronomy, Odessa State University, Shevchenko Park, 65014 Odessa, Ukraine of Astronomy, Odessa State University, Shevchenko Park, 65014 Odessa, Ukraine; Odessa Astronomical Observatory and Isaac Newton Institute of Chile, Odessa Branch, Ukraine
Department of Astronomy, Odessa State University, Shevchenko Park, 270014 Odessa, Ukraine; Isaac Newton Institute of Chile, Odessa Branch of Astronomy, Odessa State University, Shevchenko Park, 65014 Odessa, Ukraine ; Instituto Astronómico e Geofísico, Universidade de São Paulo, Av. Miguel Stefano, 4200 Agua Funda, Brasil; Odessa Astronomical Observatory and Isaac Newton Institute of Chile, Odessa Branch, Ukraine Astronomical Observatory of Odesa National University
Department of Astronomy, Odessa State University, Shevchenko Park, 270014 Odessa, Ukraine of Astronomy, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, OH 44106-7215 ; Department of Astronomy, Odessa State University, Shevchenko Park, 65014, Odessa, Ukraine of Astronomy, Odessa State University, Shevchenko Park, 270014, Odessa, Ukraine
Abundances of giants in four Galactic clusters (Sestito+, 2008)
Accurate LTE abundances for some lambda Boo stars
Accurate LTE abundances of seven well established lambda Bootis stars
An Investigation of the Double-Mode Cepheid Tu-Cassiopeiae - Part One - Atmospheric Parameters and Chemical Composition
Ba II line as Cepheid luminosity indicator. I
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