Accretion flows in the magnetospheres of VELA X-1, AO535 + 26 and HER X-1

Details Accretion flows in the magnetospheres of VELA X-1, AO535 + 26 and HER X-1 Accretion flows in the magnetospheres of VELA X-1, AO535 + 26 and HER X-1

Jul 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976natur.262..356e&link_type=abstract

Nature, vol. 262, July 29, 1976, p. 356-360. Research supported by the Alfred P. Sloan Foundation and NSF.

Astronomy and Astrophysics

Astronomy

87

Astronomical Models, Earth Magnetosphere, Mass Flow, Neutron Stars, X Ray Stars, Pulsed Radiation, Stellar Mass, Stellar Rotation, Waveforms, X Ray Sources

Scientific paper

A model for the complex pulse shapes of the long period, pulsating X-ray
sources, Vela X-1 and AO535 + 26 is suggested. The flow of accreting
matter onto these slow rotators is discussed and compared with that
expected in systems such as Her X-1 which contain a rapidly rotating
neutron star.

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