The crust screen model for the magnetic field of binary X-ray sources

Details The crust screen model for the magnetic field of binary X-ray sources The crust screen model for the magnetic field of binary X-ray sources

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...283..889z&link_type=abstract

Astronomy and Astrophysics, Vol. 283, p. 889 (1994)

Astronomy and Astrophysics

Astrophysics

14

Star: Neutron - Stars: Magnetic Field - X-Rays: Stars - Stars: Binaries: Close

Scientific paper

It is assumed that the compressed accretion matter on the crust of a neutron star with magnetic field has ferromagnetic permeability. The observed inverse correlation between field strength and accreted mass can be deduced, by means of the analytic calculation of a proposed crust screen model. The field-period relation P = 2.7 ms B5/79 is also presented, which fits for the equilibrium period line of X-ray binary sources.

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