Abstract The velocity profiles and properties of proto-magnetar winds are investigated. It is found that the corotation of wind matter with magnetic field lines significantly affects r-process nucleosynthesis and could lead to long duration γ-ray bursts and hyper-energetic supernovae.
Keywords stars: neutron— stars: winds, outflows— supernovae: general— stars: magnetic fields — nuclear reactions, nucleosynthesis, abundances
It accepts original submissions from all over the world and is internationally published and distributed by IOP