Observations of post-Newtonian timing effects in the binary pulsar PSR 1913 + 16

Details Observations of post-Newtonian timing effects in the binary pulsar PSR 1913 + 16 Observations of post-Newtonian timing effects in the binary pulsar PSR 1913 + 16

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phrvl..52.1348w&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 52, April 9, 1984, p. 1348-1350.

Physics

147

Binary Stars, Orbit Decay, Pulsars, Stellar Motions, Companion Stars, Gravitational Fields, Relativity, Stellar Mass, Stellar Radiation, Time Lag

Scientific paper

The authors report the latest results of timing measurements of the binary pulsar PSR 1913+16. Recent high-quality data have enabled them to measure the excess propagation delay of the pulsar signal caused by the gravitational field of the companion star; this result provides strong additional support for the simplest and most straightforward model of the system. The observed rate of orbital period decay is equal to 1.00±0.04 times that expected from gravitational radiation damping.

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