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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Restricted until

2037-12-31