Using the CIFIST grid of CO5BOLD 3D model atmospheres to study the effects of stellar granulation on photometric colours - II. The role of convection across the H–R diagram

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Fig. 1

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3D hydrodynamical CO⁵BOLD and 1D hydrostatic LHD model atmospheres used in this work, shown in the log g–T_eff plane (large yellow-filled circles). Different isochrones (Pietrinferni et al. 2004, 2006) indicate the approximate loci of stars in the Galactic thin and thick disk, bulge, and halo.

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