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Self-Consistency of Relativistic Observables with General Relativity in the White Dwarf-Neutron Star Binary PSR J1141-6545

ASTROPHYSICAL JOURNAL, no. 1 (2003): L49-L52

Cited: 97|Views23
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Here we report timing measurements of the relativistic binary PSR J1141 - 6545 that constrain the component masses and demonstrate that the orbital period derivative P-b = (-4 +/- 1) x 10(-13) is consistent with gravitational wave emission as described by the general theory of relativity. The mass of the neutron star and its companion are...More

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