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Accretion Models for Young Neutron Stars

Research paper by M. Ali Alpar

Indexed on: 09 Jun '03Published on: 09 Jun '03Published in: Astrophysics



Abstract

Interaction with possible fallback material, along with the magnetic fields and rotation rates at birth should determine the fates and categories of young neutron stars. This paper addresses some issues related to pure or hybrid accretion models for explaining the properties of young neutron stars.