Examples of RHD simulations of stellar surface convection

• Nordlund, Dravins (1982): first coarse incompressible solar models + spectra
• Nordlund & Stein et al. (until now): succession of improvements
• Stein, Benson (2006): huge 3D solar model

• Robinson (2004): 3D surface of subgiant star (T_eff=5000K; logg=3.37)
• Ludwig (2006): microvariability
• Collet (2007): 3D surface of red giants (T_eff=4700K, 5000K; logg=2.2; [Fe/H]=0,-1,-2,-3)
• Asida & Tuchman (1997, 2000): deep 2D giant models (T_eff=4900K, logg=2.2)
• Woodward et al. (1996): high-resolution 3D simulation of giant star envelope
• Freytag, Steffen, & Dorch (2002): mini-Betelgeuse in 3D
• Freytag & Höfner (2008): 3D AGB star