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A Model for the Double System Containing the X-Ray Pulsar Her X-1

Published online by Cambridge University Press:  14 August 2015

G. S. Bisnovatyi-Kogan
Affiliation:
Institute for Space Research, Academy of Sciences, Moscow, U.S.S.R.
B. V. Komberg
Affiliation:
Institute for Space Research, Academy of Sciences, Moscow, U.S.S.R.

Abstract

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A model for the double system with the X-ray source Her X-1 is considered. It is supposed that the central star has a sufficiently strong magnetic field for the outflow of the matter to occur in jets. When the neutron star is in the jet the optical depth τx attributable to the X-ray emission due to Compton scattering is greater than unity and the solid angle of the emitted X-radiation is broad, ∼ 180°. In the opposite case, τx < 1, there is a narrow angle of emission and the radiation falls on to the star and is not observed on the Earth. The motion of the neutron star relative to the jet is due to nonsynchronization between the orbital motion and rotation of the central star. If the duration of the whole orbit around the central star is 35 days and the dimension of the jet is about 1/3 of the orbit, then such a model explains features connected with the 35-day cycle.

Type
Part 9 / Variable X-Ray Sources
Copyright
Copyright © Reidel 1975