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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1777
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dc.contributor.authorSivaram, C-
dc.date.accessioned2007-09-13T08:56:18Z-
dc.date.available2007-09-13T08:56:18Z-
dc.date.issued1995-
dc.identifier.citationBASI, Vol. 23, No. 1, pp. 77-83en
dc.identifier.urihttp://hdl.handle.net/2248/1777-
dc.description.abstractThe significance of the binary pulsar 1913+16 in establishing evidence for gravitational radiation emission from binary systems is described. It is pointed out that the system has enabled verification of general relativity predictions to a high level of precision. This article was written on the occasion of the 1993 Physics Nobel Prize awarded to Hulse and Taylor.en
dc.format.extent551133 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1995BASI...23...77Sen
dc.subjectbinary pulsaren
dc.subjectPSR 1913-16en
dc.titleThe Hulse-Taylor binary pulsar PSR 1913+16.en
dc.typeArticleen
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