Nucleosynthesis in Classical Novae: CO versus ONe White Dwarfs
Nucleosynthesis in Classical Novae: CO versus ONe White Dwarfs
Detailed nucleosynthesis in the ejecta of classical novae has been determined for a grid of hydrodynamic nova models. The reported 14 evolutionary sequences, followed from the onset of accretion up to the explosion and ejection stages, span a range of CO and ONe white dwarf masses (0.8-1.35 M☉) and mixing …