A grid of three-dimensional stellar atmosphere models of solar metallicity. I. General properties, granulation, and atmospheric expansion
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Trampedach, Regner
Asplund, Martin
Collet, Remo
Nordland, Ake
Stein, R. F.
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IOP Publishing
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Present grids of stellar atmosphere models are the workhorses in interpreting stellar observations and determining their fundamental parameters. These models rely on greatly simplified models of convection, however, lending less predictive power to such m
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Astrophysical Journal, The
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Open Access
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