34 citations · 124 across the 10 of their papers we have counts for
6 papers · 1 filter
3D hydrodynamics simulations of a 3 core-helium burning star
Simon Blouin, Falk Herwig, Huaqing Mao +2
The inner structure of core-helium burning (CHeB) stars remains uncertain due to the yet unknown nature of mixing at the boundary of their cores. Large convective cores beyond a ba…
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…
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…
3D hydrodynamics simulations of internal gravity waves in red giant branch stars
Simon Blouin, Huaqing Mao, Falk Herwig +3
We present the first 3D hydrodynamics simulations of the excitation and propagation of internal gravity waves (IGWs) in the radiative interiors of low-mass stars on the red giant b…
3D hydrodynamic simulations of massive main-sequence stars II. Convective excitation and spectra of internal gravity waves
William Thompson, Falk Herwig, Paul R. Woodward +4
Recent photometric observations of massive stars have identified a low-frequency power excess which appears as stochastic low-frequency variability in light curve observations. We…
3D hydrodynamic simulations of massive main-sequence stars. I. Dynamics and mixing of convection and internal gravity waves
Falk Herwig, Paul R. Woodward, Huaqing Mao +6
We performed 3D hydrodynamic simulations of the inner radial extent of a star in the early phase of the main sequence and investigate core con…