3 papers
astro-ph.SR2020
Comparison of two- and three-dimensional compressible convection in a pre-main sequence star
J. Pratt, I. Baraffe, T. Goffrey +4
Extending our recent studies of two-dimensional stellar convection to 3D, we compare three-dimensional hydrodynamic simulations to identically set-up two-dimensional simulations, f…
astro-ph.SR2019
A well-balanced scheme for the simulation tool-kit A-MaZe: implementation, tests, and first applications to stellar structure
M. V. Popov, R. Walder, D. Folini +6
Characterizing stellar convection in multiple dimensions is a topic at the forefront of stellar astrophysics. Numerical simulations are an essential tool for this task. We present…
astro-ph.SR2016
Multi-dimensional structure of accreting young stars
C. Geroux, I. Baraffe, M. Viallet +6
This work is the first attempt to describe the multi-dimensional structure of accreting young stars based on fully compressible time implicit multi-dimensional hydrodynamics simula…