The Crab pulsar as a component of binary system

Details The Crab pulsar as a component of binary system The Crab pulsar as a component of binary system

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974azh....51.1339t&link_type=abstract

Astronomicheskii Zhurnal, vol. 51, Nov.-Dec. 1974, p. 1339-1341. In Russian.

Astronomy and Astrophysics

Astronomy

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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