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Accretion by rotating magnetic neutron stars. I. Flow of matter inside the magnetosphere and its implications for spin-up and spin-down of the star

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/155606· OSTI ID:5433217
We investigate the flow of accreting matter and the configuration of the magnetic field inside the magnetosphere of a rotating neutron star. We assume that the magnetic field of the star has a symmetry axis which is aligned with the rotation axis, that the accreting plasma becomes threaded by the stellar magnetic field near the magnetospheric boundary, and that the star is not a fast rotator. We show that for bright X-ray sources, flow within the Alfven surface is well described by the equations of magnetohydrodynamics and that the matter moves along field lines when viewed in the frame corotating with the star. In the case of slow rotators, matter inside the Alfven surface rotates in a sense opposite that of the net angular momentum flux toward the star. We also study the torque exerted on the star by the accreting matter and the flow of energy within the magnetosphere and the transition region at the magnetospheric boundary, when the star accretes matter from a disk. Finally, we comment briefly on the implications of our results for pulsating X-ray sources.
Research Organization:
Department of Physics, University of Illinois at Urbana-Champaign
OSTI ID:
5433217
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 217:2; ISSN ASJOA
Country of Publication:
United States
Language:
English