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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1902
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dc.contributor.authorMcConnell, D.-
dc.contributor.authorDeshpande, A.A.-
dc.contributor.authorConnors, T.-
dc.contributor.authorAbles, J.G.-
dc.date.accessioned2007-01-23T06:27:38Z-
dc.date.available2007-01-23T06:27:38Z-
dc.date.issued2004-03-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2004, Vol.348, Issue 4, p1409-1414.en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2289/1902-
dc.descriptionRestricted Access. An open access version is available at arXiv.org.en
dc.description.abstractWe have used the Australia Telescope Compact Array to seek the integrated radio flux from all the pulsars in the core of the globular cluster 47 Tucanae. We have detected an extended region of radio emission and have calibrated its flux against the flux distribution of the known pulsars in the cluster. We find the total 20-cm radio flux from the pulsars in the cluster to be S= 2.0 +/- 0.3 mJy. This implies the lower limit to the radio luminosity distribution to be minL1400= 0.4 mJy kpc2 and the size of the observable pulsar population to be N<~ 30.en
dc.format.extent8338 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherBlackwell Publishing for the Royal Astronomical Societyen
dc.relation.urihttp://arxiv.org/abs/astro-ph/0312107en
dc.relation.urihttp://dx.doi.org/10.1111/j.1365-2966.2004.07447.xen
dc.rights(2004) Royal Astronomical Societyen
dc.subjectpulsars: generalen
dc.subjectglobular clusters: individual: 47 Tucanaeen
dc.titleThe radio luminosity distribution of pulsars in 47 Tucanaeen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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