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A new test of general relativity - Gravitational radiation and the binary pulsar PSR 1913+16
, 1982Observations of pulse arrival times from the binary pulsar PSR 1913+16 between 1974 September and 1981 March are now sufficient to yield a solution for the component masses and the absolute size of the orbit.
J. Taylor, J. Weisberg
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Optical identification of binary pulsars
Advances in Space Research, 1988Abstract Of the nearly 500 known pulsars, only seven pulsars are in binary systems. In this article, I review the identification of binary pulsars with emphasis on the critical and unique information provided by optical observations. Optical observations have provided: (i) basic conformation of the stellar evolution acenarios and (ii) observational ...
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LIMITING BRANEWORLDS WITH THE BINARY PULSAR
The Tenth Marcel Grossmann Meeting, 2006Ruth Durrer, Philippe Kocian
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