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In this talk we review the basic assumptions and physics covered by classical1D LTE model atmospheres. We will focus on ATLAS and MARCS models of F-G-Kstars and describe what resources are available through the web, both in termsof codes and model-atmosphere grids. We describe the advances made inhydrodynamical simulations of convective stellar atmospheres with the CO5BOLDcode and what grids and resources are available, with a prospect of what willbe available in the near future.

LTE model atmopsheres MARCS, ATLAS and CO5BOLD