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Cited article:

Performance of high-order Godunov-type methods in simulations of astrophysical low Mach number flows

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Turbulent dynamo action and its effects on the mixing at the convective boundary of an idealized oxygen-burning shell

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Simulations of common-envelope evolution in binary stellar systems: physical models and numerical techniques

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A finite-volume scheme for modeling compressible magnetohydrodynamic flows at low Mach numbers in stellar interiors

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Dynamics in a stellar convective layer and at its boundary: Comparison of five 3D hydrodynamics codes

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Well-balanced treatment of gravity in astrophysical fluid dynamics simulations at low Mach numbers

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https://doi.org/10.1051/0004-6361/202140653

Multidimensional low-Mach number time-implicit hydrodynamic simulations of convective helium shell burning in a massive star

L. Horst, R. Hirschi, P. V. F. Edelmann, R. Andrássy and F. K. Röpke
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Fully compressible simulations of waves and core convection in main-sequence stars

L. Horst, P. V. F. Edelmann, R. Andrássy, et al.
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60Fe in core-collapse supernovae and prospects for X-ray and gamma-ray detection in supernova remnants

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https://doi.org/10.1093/mnras/stz536

Dependence of convective boundary mixing on boundary properties and turbulence strength

A Cristini, R Hirschi, C Meakin, et al.
Monthly Notices of the Royal Astronomical Society 484 (4) 4645 (2019)
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Sensitivity of gravito-inertial modes to differential rotation in intermediate-mass main-sequence stars

T. Van Reeth, J. S. G. Mombarg, S. Mathis, et al.
Astronomy & Astrophysics 618 A24 (2018)
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Astrophysics with Radioactive Isotopes

Friedrich-Karl Thielemann, Roland Diehl, Alexander Heger, Raphael Hirschi and Matthias Liebendörfer
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https://doi.org/10.1007/978-3-319-91929-4_4