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Paper: 3D Anelastic Simulations of Convection in Massive Stars
Volume: 293, 3D Stellar Evolution
Page: 147
Authors: Kuhlen, M.; Woosley, W. E.; Glatzmaier, G. A.
Abstract: After briefly describing the anelastic approximation and Glatzmaier's code, we present results from our preliminary studies of core convection during the hydrogen burning phase of a 15 Msun star, as well as our most recent results concerning convection in the oxygen shell of a 25 Msun star.
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