Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
St. Petersburg and MPA
St. Petersburg & MSSSO
the Astronomical Institute of the St. Petersburg University
Astronomical Institute of the St. Petersburg University, Bibliotechnaja Pl. 2, Petrodvorets, 198904 St. Petersburg, Russia; Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, D-85740 Garching bei München, Germany
Max-Planck-Inst für Astrophysik, Garching bei München, Germany
University of Victoria
The Ohio State University
Univ. St. Petersburg & MPA
University of Victoria, Canada
Sobolev Astronomical Institute, St. Petersburg University, St. Petersburg;
Max-Planck-Institut f. Astrophysik, Garching, Germany and St. Petersburg University, Russia
Astronomical Institute, St. Petersburg University, Bibliotechnaya Pl. 2, Petrodvorets, 198904 St Petersburg, Russia
Department of Physics and Astronomy, University of Victoria, P.O. Box 3055, Victoria, BC V8W 3P6, Canada; On leave from Sobolev Astronomical Institute, St. Petersburg University, Universitetsky Pr. 28, Petrodvorets, 198504 St. Petersburg, Russia. of Physics and Astronomy, University of Victoria, P.O. Box 3055, Victoria, BC, V8W 3P6, Canada; On leave from Sobolev Astronomical Institute, St. Petersburg University, Universitetsky Pr. 28, Petrodvorets, 198504 St. Petersburg, Russi; Department of Physics and Astronomy, Dartmouth College, 6127 Wilder Laboratory, Hanover, NH 03755-3528 Astronomical Institute, St Petersburg University, Universitetsky Pr. 28, Petrodvorets, 198504 St Petersburg, Russia; Institute of Astronomy, The Observatoires, Madingley Road, Cambridge CB3 0HA
Department of Physics and Astronomy, University of Victoria, P.O. Box 3055, Victoria, BC V8W 3P6, Canada; Max Planck Institute for Astrophysics, Karl-Schwarzschild-Strasse 1, Postfach 1317, D-85741 Garching bei München, Germany of Physics and Astronomy, University of Victoria, P.O. Box 3055, Victoria, BC V8W 3P6, Canada
23Na production in intermediate-mass MS stars with turbulent diffusive mixing.
3He in stars of low and intermediate mass
3He-Driven Mixing in Low-Mass Red Giants: Convective Instability in Radiative and Adiabatic Limits
A contribution of 26Al to the O-Al anticorrelation in globular cluster red giants
A discussion of self-pollution mechanisms
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