Showing 1–20 of 78 results
/ Date/ Name
Aug 21, 2019The Progenitors of Calcium-Strong TransientsMay 12, 2022Binary Interaction Dominates Mass Ejection in Classical NovaeAug 8, 2023The Q Branch Cooling Anomaly Can Be Explained by Mergers of White Dwarfs and Subgiant StarsAug 19, 2011The Long-Term Evolution of Double White Dwarf MergersJun 20, 2009Helium White Dwarfs in Cataclysmic VariablesFeb 11, 2010Thermonuclear .Ia Supernovae from Helium Shell Detonations: Explosion Models and ObservablesMay 14, 2008The Effect of Composition on Nova IgnitionsFeb 6, 2025The Evolution of Hypervelocity Supernova Survivors and the Outcomes of Interacting Double White Dwarf BinariesMay 29, 2013The Ignition of Carbon Detonations via Converging Shock Waves in White DwarfsFeb 17, 2015Every interacting double white dwarf binary may mergeOct 20, 2016Wait for it: Post-supernova winds driven by delayed radioactive decaysJun 6, 2017Sub-Chandrasekhar-mass white dwarf detonations revisitedFeb 12, 2013Circumstellar absorption in double detonation Type Ia supernovaeMay 29, 2024Almost All Carbon/Oxygen White Dwarfs Can Host Double DetonationsAug 27, 2021Multi-Dimensional Radiative Transfer Calculations of Double Detonations of Sub-Chandrasekhar-Mass White DwarfsMar 22, 2007Faint Thermonuclear Supernovae from AM Canum Venaticorum BinariesMar 3, 2009Unstable Helium Shell Burning on Accreting White DwarfsFeb 16, 2021Non-Local Thermodynamic Equilibrium Radiative Transfer Simulations of Sub-Chandrasekhar-Mass White Dwarf DetonationsOct 25, 2017The Evolution of the Type Ia Supernova Luminosity FunctionFeb 2, 2007Thermally Stable Nuclear Burning on Accreting White Dwarfs