On 'An exact solution of Haugan's binary pulsar equation of motion'

Details On 'An exact solution of Haugan's binary pulsar equation of motion' On 'An exact solution of Haugan's binary pulsar equation of motion'

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...333l..23h&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 333, Oct. 1, 1988, p. L23, L24. CNRS-supported research.

Astronomy and Astrophysics

Astrophysics

Binary Stars, Pulsars, Stellar Motions, Newton Theory, Orbital Mechanics, Relativity, Two Body Problem

Scientific paper

The analysis of the equation for the relative orbit of a post-Newtonian two-body system published recently by Weinstein and Mor (45.066.104) does not properly incorporate the Newtonian limit. As a result, the solution they derive is of no use for dealing with the motion of the binary pulsar. The claim that the form of their solution implies that earlier treatments of post-Newtonian orbital motion have missed significant effects is mistaken.

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