The Crab Nebula pulsar as a binary-system component

Details The Crab Nebula pulsar as a binary-system component The Crab Nebula pulsar as a binary-system component

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sva....18..798t&link_type=abstract

(Astronomicheskii Zhurnal, vol. 51, Nov.-Dec. 1974, p. 1339-1341.) Soviet Astronomy, vol. 18, May-June 1975, p. 798, 799. Trans

Astronomy and Astrophysics

Astronomy

8

Binary Stars, Crab Nebula, Pulsars, Stellar Motions, X Ray Sources, Astronomical Models, Eccentric Orbits, Neutron Stars, Orbital Elements, Stellar Rotation, Variable Stars

Scientific paper

The idea is developed that the Crab pulsar is a component of a binary system with a large orbital eccentricity. The orbital parameters are estimated from the braking index (change due to the Doppler effect) of neutron star rotation. A similar model is proposed for explaining flaring X-ray sources such as GX-333 + 25 (Cen XR-4). The influence of precession on the experimental braking index of neutron star rotation is considered.

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