2 papers
astro-ph.SR2024
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.SR2024
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…