The Hulse-Taylor binary pulsar PSR 1913+16.

dc.contributor.author	Sivaram, C
dc.date.accessioned	2007-09-13T08:56:18Z
dc.date.available	2007-09-13T08:56:18Z
dc.date.issued	1995
dc.identifier.citation	BASI, Vol. 23, No. 1, pp. 77-83	en
dc.identifier.uri	http://hdl.handle.net/2248/1777
dc.description.abstract	The 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.extent	551133 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1995BASI...23...77S	en
dc.subject	binary pulsar	en
dc.subject	PSR 1913-16	en
dc.title	The Hulse-Taylor binary pulsar PSR 1913+16.	en
dc.type	Article	en