3D Anelastic Simulations of Convection in Massive Stars

Details 3D Anelastic Simulations of Convection in Massive Stars 3D Anelastic Simulations of Convection in Massive Stars

2002-10-25

arxiv.org/abs/astro-ph/0210557v1

Astronomy and Astrophysics

Astrophysics

10 pages, 4 very low resolution color eps figures. Contributed talk given at 2002 Stellar Evolution Workshop at LLNL. Higher r

Scientific paper

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.

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