3D Anelastic Simulations of Convection in Massive Stars
arXiv:astro-ph/0210557
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 solar mass star, as well as our most recent results concerning convection in the oxygen shell of a 25 solar mass star.
10 pages, 4 very low resolution color eps figures. Contributed talk given at 2002 Stellar Evolution Workshop at LLNL. Higher resolution figures can be obtained at: http://www.supersci.org