21 citations · 26 across the 3 of their papers we have counts for
3 papers
astro-ph.SR2023★ 2 cited
3D hydrodynamic simulations of massive main-sequence stars. III. The effect of radiation pressure and diffusion leading to a 1D equilibrium model
Huaqing Mao, Paul Woodward, Falk Herwig +4
We present 3-D hydrodynamical simulations of core convection with a stably stratified envelope of a \unit{25}{\Msun} star in the early phase of the main-sequence. We use the explic…
astro-ph.SR2023★ 3 cited
3D hydrodynamics simulations of core convection in supermassive main-sequence stars
Simon Blouin, Huaqing Mao, Tyrone E. Woods +3
Supermassive stars are Population III stars with masses exceeding that could be the progenitors of the first supermassive black holes. Their interiors are in a re…
astro-ph.SR2021★ 21 cited
Dynamics in a stellar convective layer and at its boundary: Comparison of five 3D hydrodynamics codes
R. Andrassy, J. Higl, H. Mao +18
Our ability to predict the structure and evolution of stars is in part limited by complex, 3D hydrodynamic processes such as convective boundary mixing. Hydrodynamic simulations he…