Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
University of Vienna
Astronomy Unit, School of Mathematical Sciences, Queen Mary, University of London, UK;
Institute for Astronomy, University of Vienna
Garching / Germany
P.I. M.-L. Dubernet
Max-Planck-Institute for Astrophysics, Garching
Max-Planck-Institute for Astrophysics, Garching, Germany
Institute for Astronomy, University Vienna, Türkenschanzstrasse 17, 1180 Vienna, Austria for Astronomy, University of Vienna, Türkenschanzstrasse 17, A-1180 Vienna, Austria
Max-Planck-Institute for Astrophysics, Karl-Schwarzschild Str. 1, D-85748 Garching bei München, Germany for Astrophysics, Garching bei München, Germany
Max-Planck-Institute for Astrophysics, Karl-Schwaarzschild-Str. 1, D-85741 Garching bei München, Germany for Astrophysics, Karl-Schwarzschild Str. 1, D-85741 Garching bei München, Germany
Institute for Astronomy, University of Vienna, Türkenschanzstrasse 17, 1180 Wien, Austria
Astronomy Unit, School of Mathematical Sciences, Queen Mary, University of London, Mile End Road, London E1 4NS; Institut für Astronomie, Universität Wien, Türkenschanzstrasse 17, A-1180 Wien, Austria
Inst. for Astronomy, University of Vienna, Turkenschanzstr. 17, A-1180 Vienna, Austria for Astrophysics, Karl-Schwarzschild-Str. 1, 85741 Garching bei München, Germany
Institute for Astronomy, University of Vienna, Tuerkenschanzstrasse 17, A-1180 Vienna, Austria for Astronomy, University of Vienna, Türkenschanzstrasse 17, A-1180 Vienna, Austria Unit, School of Mathematical Sciences, Queen Mary, University of London Mile End Road, London E1 4NS, UK ; Institut für Astromomie Universität Wien, Türkenschanzstrasse 17, 1180 Vienna, Austria for Astronomy, University of Vienna, A-1180 Vienna, Austria
Faculty of Mathemati
(Erratum) Abundance analysis of roAp stars.
3D stellar atmospheres for stellar structure models and asteroseismology
A closure model for turbulent convection. Application to the excitation of p modes
A closure model with plumes I. The solar convection
A closure model with plumes II. Application to the stochastic excitation of stellar p modes
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