Towards a self-consistent model of the convective core boundary in upper main sequence stars. I. 2.5D and 3D simulations

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SEEK ID: https://publications.h-its.org/publications/1930

DOI: 10.1051/0004-6361/202347407

Research Groups: Stellar Evolution Theory

Publication type: Journal

Journal: Astronomy and Astrophysics

Citation: A&A 683:A97

Date Published: 1st Mar 2024

Registered Mode: imported from a bibtex file

Authors: R. Andrassy, G. Leidi, J. Higl, P. V. F. Edelmann, F. R. N. Schneider, F. K. Röpke

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Andrassy, R., Leidi, G., Higl, J., Edelmann, P. V. F., Schneider, F. R. N., & Röpke, F. K. (2024). Towards a self-consistent model of the convective core boundary in upper main sequence stars. In Astronomy & Astrophysics (Vol. 683, p. A97). EDP Sciences. https://doi.org/10.1051/0004-6361/202347407
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