Three-dimensional modelling of proton ingestion episodes in low-mass stars
We have modelled a dual shell flash (DSF) in a low-metallicity 1.5M ȯ AGB star using the 3-dimensional hydrodynamic program "Djehuty", observing how the evolution of these events compares to 1-dimensional models, which are hypothesised to be inaccurate d
|Collections||ANU Research Publications|
|Source:||Proceedings of Science|
|01_Heap_Three-dimensional_modelling_of_2013.pdf||1.49 MB||Adobe PDF||Request a copy|
|02_Heap_Three-dimensional_modelling_of_2013.pdf||87.88 kB||Adobe PDF||Request a copy|
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