The importance of gravitational self-field effects in binary systems with compact objects. I - The 'static two-body problem' and the attraction law in a post-Newtonian approximation of general relativity. II - The 'static two-body problem' and the attracti

Details The importance of gravitational self-field effects in binary systems with compact objects. I - The 'static two-body problem' and the attraction law in a post-Newtonian approximation of general relativity. II - The 'static two-body problem' and the attracti The importance of gravitational self-field effects in binary systems with compact objects. I - The 'static two-body problem' and the attraction law in a post-Newtonian approximation of general relativity. II - The 'static two-body problem' and the attracti

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978gregr...9..809r&link_type=ejournal

General Relativity and Gravitation, vol. 9, Sept. 1978, p. 809-833.

Astronomy and Astrophysics

Astronomy

3

Astronomical Models, Gravitational Effects, Gravitational Fields, Relativity, Two Body Problem, Approximation, Binary Stars, Mathematical Models, Newton Theory

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