Accretion onto magnetized neutron stars: Magnetospheric structure and stability

Details Accretion onto magnetized neutron stars: Magnetospheric structure and stability Accretion onto magnetized neutron stars: Magnetospheric structure and stability

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aipc..115..215a&link_type=abstract

AIP Conference Proceedings, Volume 115, pp. 215-234 (1984).

Physics

28

X-Ray Sources, X-Ray Bursts, Radio Sources, X-Ray Binaries, Late Stages Of Stellar Evolution

Scientific paper

A summary is given of the magnetospheric physics of accreting magnetized neutron stars. The role of hydromagnetic instabilities is described, with particular attention to the formation of polar caps in spherical and disk on, and to the origin of spin down torques in a centrigugally driven stellar wind, when the accretion is from a disk. The most elementary consequences for formation of the emergent spectrum are also discussed.

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