Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1127
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dc.contributor.authorSrinivasan, G.-
dc.contributor.authorBhattacharya, D.-
dc.date.accessioned2006-01-09T06:06:36Z-
dc.date.available2006-01-09T06:06:36Z-
dc.date.issued1989-09-05-
dc.identifier.citationCurrent Science, 1989, Vol. 58, p953-954.en
dc.identifier.issn0011-3891-
dc.identifier.urihttp://hdl.handle.net/2289/1127-
dc.description.abstractIt is argued that the measured mass of the binary millisecond pulsar PSR 0021-72A provides a strong evidence that a rapidly spinning neutron star may drastically curtail the X-ray lifetime of a binary system.en
dc.format.extent142372 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciences, Bangalore, India.en
dc.rightsIndian Academy of Sciences, Bangalore, India.en
dc.titleOn the lifetime of low mass x-ray binariesen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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