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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1412
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dc.contributor.authorNarlikar, J. V-
dc.date.accessioned2007-03-14T06:14:52Z-
dc.date.available2007-03-14T06:14:52Z-
dc.date.issued1990-
dc.identifier.citationBASI, Vol. 18, pp. 171-176en
dc.identifier.urihttp://hdl.handle.net/2248/1412-
dc.description.abstractConceptual and observational issues involved in using binary stars for tests of theories of gravity are discussed. Individual binary star systems that offer the most suitable opportunities for such testing are examined, and difficulties associated with claims that certain binary pulsar observations fit theoretical predictions are reviewed. The approximate procedure that is followed by theoreticians in dealing with the strong gravity case is considereden
dc.format.extent195444 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectBinary strasen
dc.subjectGravitational theoryen
dc.titleBinary stars as tests of gravity theoryen
dc.typeBooken
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