"au:"W. D. Arnett"" — arXiv2 SearchShowing 1–9 of 9 results
/ Date/ Name
Jul 7, 2022Realistic 3D hydrodynamics simulations find significant turbulent entrainment in massive starsNov 26, 2012Hydrodynamic Studies of the Evolution of Recurrent, Symbiotic, and Dwarf Novae: The White Dwarf Components are Growing in MassOct 22, 2012Theoretical Studies of Accretion of Matter onto White Dwarfs and the Single Degenerate Scenario for Supernovae of Type IaMay 23, 20233D stellar evolution: hydrodynamic simulations of a complete burning phase in a massive starMay 31, 20243D simulations of convective shell Neon-burning in a massive starNov 1, 2021Dynamics in a stellar convective layer and at its boundary: Comparison of five 3D hydrodynamics codesDec 12, 2025The Impact of Initial Mass Dependent Convective Boundary Mixing on the Structure and Fates of Massive StarsMar 10, 2021Convective core entrainment in 1D main sequence stellar modelsDec 15, 2015Towards 21st Century Stellar Models: Star Clusters, Supercomputing, and Asteroseismology