Speaker
John Lattanzio
(Monash University)
Description
We present fully three dimensional models of the core helium flash in low mass stars.
These hydordynamical models show that the simple 1D hydrostatic models are not too
misleading! New results, for rotating models, will be reported.
Author
John Lattanzio
(Monash University)
Co-authors
Dr
David Dearborn
(Lawrence Livermore National Laboratory)
Dr
Don Dossa
(Lawrence Livermore National Laboratory)
Dr
Peter Eggleton
(Lawrence Livermore National Laboratory)
