Accretion Models for Young Neutron Stars

Details Accretion Models for Young Neutron Stars Accretion Models for Young Neutron Stars

2003-06-09

arxiv.org/abs/astro-ph/0306179v1

Astronomy and Astrophysics

Astrophysics

6 pages, to appear in the proceedings of the workshop "Pulsars, AXPs and SGRs observed with BeppoSAX and other Observatories"

Scientific paper

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.

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