Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5709
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dc.contributor.authorSafonova, M-
dc.contributor.authorRahvar, S-
dc.date.accessioned2012-02-28T16:12:53Z-
dc.date.available2012-02-28T16:12:53Z-
dc.date.issued2007-04-
dc.identifier.citationInternational Astronomical Union Symposium; No. 238, pp. 439-440en
dc.identifier.urihttp://hdl.handle.net/2248/5709-
dc.description.abstractGlobular clusters have been long predicted to host intermediate-mass black holes (IMBHs) in their centres. The growing evidence that some/all Galactic globular clusters (GCs) could harbour middle range (102 – 104Mxs2299) black holes, just as galaxies do, stimulates the searches and the development of new methods for proving their existence. Here we propose another method of detection – the microlensing of the cluster stars by the central BH.en
dc.language.isoenen
dc.publisherCambridge University Pressen
dc.relation.urihttp://dx.doi.org/10.1017/S1743921307005844en
dc.rights© International Astronomical Unionen
dc.subjectGravitational lensingen
dc.subject(Galaxy:) globular clusters: generalen
dc.titleDetection of IMBHs from microlensing in globular clustersen
dc.typeArticleen
Appears in Collections:IIAP Publications

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