3D1D hydro-nucleosynthesis simulations. I. Advective-reactive post-processing method and its application to H ingestion into He-shell flash convection in rapidly accreting white dwarfs

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SEEK ID: https://publications.h-its.org/publications/1223

DOI: 10.1093/mnras/stab500

Research Groups: Physics of Stellar Objects

Publication type: Journal

Journal: Monthly Notices of the Royal Astronomical Society

Citation: Monthly Notices of the Royal Astronomical Society,stab500

Date Published: 20th Feb 2021

Registered Mode: by DOI

Authors: David Stephens, Falk Herwig, Paul Woodward, Pavel Denissenkov, Robert Andrassy, Huaqing Mao

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Stephens, D., Herwig, F., Woodward, P., Denissenkov, P., Andrassy, R., & Mao, H. (2021). 3D1D hydro-nucleosynthesis simulations – I. Advective–reactive post-processing method and its application to H ingestion into He-shell flash convection in rapidly accreting white dwarfs. In Monthly Notices of the Royal Astronomical Society (Vol. 504, Issue 1, pp. 744–760). Oxford University Press (OUP). https://doi.org/10.1093/mnras/stab500
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Created: 24th Feb 2021 at 13:12

Last updated: 5th Mar 2024 at 21:24

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