Binary Pulsars, General Relativity and Light-Time Effects

Details Binary Pulsars, General Relativity and Light-Time Effects Binary Pulsars, General Relativity and Light-Time Effects

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..335..215s&link_type=abstract

The Light-Time Effect in Astrophysics, Proceedings of ASP Conference Series, Vol. 335, held in Brussels 19-22 July 2004. Edited

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

Binary pulsars are extremely stable and most accurate clocks in orbit. They allow the determination of neutron-star masses and provide excellent tests for general relativity theories. This paper reviews aspects of pulsar O-C analysis and compares with O-C applications in classic stellar astrophysics. Pulsar studies are a school example of how, through increasing accuracy in the observational O term, the associated calculated C term leads to increasingly complex theoretical formalisms in the O-C investigation.

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