Nonstationary accretion onto neutron stars - Some constraints and consequences

Details Nonstationary accretion onto neutron stars - Some constraints and consequences Nonstationary accretion onto neutron stars - Some constraints and consequences

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...139....7m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 139, no. 1, Oct. 1984, p. 7-14.

Astronomy and Astrophysics

Astrophysics

14

Accretion Disks, Magnetohydrodynamic Stability, Neutron Stars, Pulsars, Stellar Mass Accretion, X Ray Sources, Binary Stars, Constraints, Heao 1, Magnetic Stars, Radiation Pressure, Stellar Luminosity, Stellar Models

Scientific paper

The model of highly nonstationary inhomogeneous accretion onto magnetized neutron stars presently discussed is noted to allow super-Eddington luminosities. The consequences yielded by the model are subject to observational testing. The model is judged to be most completely justifiable if nonlinear (and perhaps self-excited) instabilities can occur at the inner edge of the accretion disk. The present considerations are based on HEAO-1 pulse-to-pulse variation measurements of Her X1.

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