Radiation hydrodynamics simulations of stellar atmospheres

including the top of the convection zone and the atmosphere above

• Model atmospheres
  • Spectra > abundances (solar-type stars: F to M; low metallicities; white dwarfs)
  • Interferometric visibilities, lightcurves (red supergiants)
• Waves, shocks (Sun: p & g modes, molecules; AGB stars: dust)
• Overshoot, mixing (brown dwarfs: dust; A-type stars: diffusion)
• Magnetic fields (Sun)