- Poster presented at the 11th Cambridge Workshop on
- SPIE: Astronomical Telescopes and Instrumentation, 22-28 August 2002, Waikoloa, Hawaii USA
- Simulations observational
- Poster presented at the 76th Annual Meeting of the Astronomische Gesellschaft
- Conclusions ffl By no choice of ff can the local mixing length theory reproduce the velocity
- Poster presented at the ``Jahrestagung der Astronomischen Gesellschaft''
- Supergiant: global model I rms =0.376 %
- Poster presented at the Workshop on Stellar Structure
- Poster presented at the 12th Cambridge Workshop on \Cool Stars, Stellar Systems, and the Sun"
- Poster presented at the Joint European and National Astronomical Meeting, JENAM 2001
- SYNTHETIC LINE PROFILES FROM NUMERICAL SIMULATIONS OF A RED SUPERGIANT Bernd Freytag 12 , Michelle MizunoWiedner 2 , Bengt Gustafsson 2
- Poster presented at the ``Jahrestagung der Astronomischen Gesellschaft''
- Haisch B., Schmitt J.H.M.M., Rosso C., 1991, ApJL 383, 1518 Ludwig H.G., Freytag B., Steffen M., Wagenhuber J., 1995, in ``Stellar Evolution
- 1D wind model: sinusoidal piston
- SIMULATIONS OF MAGNETOHYDRODYNAMICS AND CO FORMATION FROM THE CONVECTION ZONE TO THE CHROMOSPHERE
- Poster presented at the EuroWinter School \Observing with the VLTI"
- Title : will be set by the publisher Editors : will be set by the publisher
- Poster presented at the Workshop on \Stellar Atmosphere Modeling"
- Model T eff Depth Boundary of z(v rms = Bottom Velocity logg instability 100 m/s) of model Scale Height
- Poster presented at the Cool Stars 13 workshop, 2004-07-05..09, Hamburg, Germany
- # MS, AIP, 2004 Poster presented at the AG Summer Meeting ``Cool Stars, Stellar Systems and the Sun 13'', 5 9 July 2004, Hamburg 3D Simulation of Surface Convection and
- Conclusions ffl By no choice of ff the local mixing length theory can re
- CONVECTION, ATMOSPHERES AND WINDS OF RED SUPERGIANT STARS E. Josselin1
- Convection Cells in a 3D Hydrodynamical Model of Sigurur Finnsson
- SweGrid Seminar 2003-04-09 Radiation Hydrodynamics Simulations
- THE SHOCK-PATTERNED SOLAR CHROMOSPHERE IN THE LIGHT OF ALMA S. Wedemeyer-Bohm1
- 3D SIMULATION OF CONVECTION AND SPECTRAL LINE FORMATION IN A-TYPE STARS M. Steffen1
- Typical Scales of Structures in Numerical Models of Betelgeuse Bernd Freytag & Sigurur Finnsson
- Radiation hydrodynamics simulations of the solar chromosphere
- Poster presented at the ``Jahrestagung der Astronomischen Gesellschaft''
- Poster presented at the 77th Annual Meeting of the Astronomische Gesellschaft
- Modelling the Entire Atmosphere of Betelgeuse with 3D Simulations Bernd Freytag & Michelle MizunoWiedner
- 13 Danksagung Meinem Doktorvater Prof. Dr. Hartmut Holweger danke ich f ur die interessante The
- A calibration of the mixinglength for solartype stars based on hydrodynamical models of stellar surface
- variation of the radiative flux) has an effect on the temperature gradient. The relative contributions of the individual fluxes are not universal but depend on
- Poster presented at the \International Scienti c Meeting of the Astronomische Gesellschaft"
- Dynamic Model Atmospheres of Cool Giants Susanne Hofner 1;2 , Rita Gautschy-Loidl 4 , Bernhard Aringer 3 , Walter
- Treatment of the superadiabatic convection in low--mass metal--poor stars from realistic hydrodynamics simulations
- MAGNETOHYDRODYNAMIC SIMULATION FROM THE CONVECTION ZONE TO THE CHROMOSPHERE
