3D Anelastic Simulations of Convection in Massive Stars

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dc.creatorKuhlen, Michael
dc.creatorWoosley, Stan E.
dc.creatorGlatzmaier, Gary A.
dc.date2002-10-25
dc.date.accessioned2026-07-07T02:05:50Z
dc.date.available2026-07-07T02:05:50Z
dc.descriptionAfter 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.
dc.description10 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
dc.identifierhttps://arxiv.org/abs/astro-ph/0210557
dc.identifierhttp://arxiv.org/abs/astro-ph/0210557
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5225
dc.subjectAstrophysics
dc.title3D Anelastic Simulations of Convection in Massive Stars
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