Showing 1–19 of 19 results
/ Date/ Name
Jan 6, 2023A study of convective core overshooting as a function of stellar mass based on two-dimensional hydrodynamical simulationsFeb 1, 2022Two-dimensional simulations of solar-like models with artificially enhanced luminosity. II. Impact on internal gravity wavesJan 1, 2022Local heating due to convective overshooting and the solar modelling problemSep 5, 2019A well-balanced scheme for the simulation tool-kit A-MaZe: implementation, tests, and first applications to stellar structureMar 10, 2020Comparison of two- and three-dimensional compressible convection in a pre-main sequence starJul 29, 2017Lithium depletion in solar-like stars: effect of overshooting based on realistic multi-dimensional simulationsFeb 10, 2016Multi-dimensional structure of accreting young starsAug 21, 2018On the AGB stars of M 4: A robust disagreement between spectroscopic observations and theoryJun 23, 2016Spherical-shell boundaries for two-dimensional compressible convection in a starNov 1, 2021Dynamics in a stellar convective layer and at its boundary: Comparison of five 3D hydrodynamics codesOct 31, 2016Benchmarking the Multi-dimensional Stellar Implicit Code MUSICJun 15, 2017Extreme value statistics for two-dimensional convective penetration in a pre-Main Sequence starDec 10, 2019The Aarhus Red Giants Challenge I: Stellar structures in the red giant branch phaseFeb 7, 2020The Aarhus red giants challenge II. Stellar oscillations in the red giant branch phaseSep 2, 2021Two-dimensional simulations of solar-like models with artificially enhanced luminosity -- I. Impact on convective penetrationMay 9, 2022Impact of radial truncation on global 2D hydrodynamic simulations for a Sun-like modelApr 5, 2023Two-dimensional simulations of internal gravity waves in a 5 $M_{\odot}$ Zero-Age-Main-Sequence modelFeb 11, 2013The Asymptotic Giant Branches of GCs: Selective Entry OnlyDec 15, 2015Towards 21st Century Stellar Models: Star Clusters, Supercomputing, and Asteroseismology