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Compulsory Deep Mixing of 3He and CNO Isotopes in the Envelopes of low-mass Red Giants
Peter P. Eggleton, David S. P. Dearborn, John C. Lattanzio
Three-dimensional stellar modeling has enabled us to identify a deep-mixing mechanism that must operate in all low mass giants. This mixing process is not optional, and is driven b…
Three Dimensional Simulations of the Core Helium Flash - with Rotation
John Lattanzio, David Dearborn, Peter Eggleton +1
We continue our study of the core helium flash using the three dimensional hydrodynamics code Djehuty. Continuing from earlier calculations, we now take relaxed 3D configurations a…
3D Numerical Experimentation on the Core Helium Flash of low-mass Red Giants
David S. P. Dearborn, John C. Lattanzio, Peter P. Eggleton
We model the core helium flash in a low-mass red giant using Djehuty, a fully three-dimensional (3D) code. The 3D structures were generated from converged models obtained during th…