Three-dimensional Hydrodynamical Simulations of a Proton Ingestion Episode in a Low-metallicity Asymptotic Giant Branch Star
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Stancliffe, Richard
Dearborn, David
Lattanzio, John
Heap, Stuart
Campbell, S
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IOP Publishing
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We use the three-dimensional (3D) stellar structure code DJEHUTY to model the ingestion of protons into the intershell convection zone of a 1 M ⊙ asymptotic giant branch star of metallicity Z = 10 -4. We have run two simulations: a low-resolution one of
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Astrophysical Journal, The
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2037-12-31
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