Gravitational light deflection effects in eclipsing binary pulsars

Details Gravitational light deflection effects in eclipsing binary pulsars Gravitational light deflection effects in eclipsing binary pulsars

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...303..601g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 303, April 15, 1986, p. 601-604.

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5

Eclipsing Binary Stars, Gravitational Effects, Pulsars, Relativistic Effects, Stellar Radiation, X Ray Binaries, Pulsed Radiation, Stellar Orbits, Time Lag

Scientific paper

A study of the general relativistic deflection of light in an idealized eclipsing binary pulsar system is performed, which indicates that the pulse train of the pulsar is differentially delayed through the course of the orbit in a way distinct from other observed delays. The effect is calculated for the Hercules X-1-HZ Herculis system because it most closely resembles the idealized system used to solve the problem. It is shown to be marginally detectable at present for Her X-1, and may possibly be more evident in other eclipsing X-ray binary pulsars.

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