Centrifugally exhausting discs - an inverse process of disc-like accretion

Details Centrifugally exhausting discs - an inverse process of disc-like accretion Centrifugally exhausting discs - an inverse process of disc-like accretion

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.237...49k&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 237, March 1, 1989, p. 49-66.

Astronomy and Astrophysics

Astronomy

3

Accretion Disks, Magnetic Stars, Stellar Mass Ejection, Stellar Rotation, Supernova 1987A, Angular Momentum, Magnetohydrodynamic Flow, Neutron Stars, Steady State

Scientific paper

A disc-like mass-loss process from rapidly rotating highly magnetized objects is studied. A nearly self-consistent set of analytic expressions is presented as a solution to the steady-state resistive MHD equations which are fairly simplified by the thin disk assumption. The possibility of finding these disks around young neutron stars is discussed with reference to SN 1987A.

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