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dc.contributor.authorSafonova, M-
dc.contributor.authorRahvar, S-
dc.identifier.citationInternational Astronomical Union Symposium; No. 238, pp. 439-440en
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.publisherCambridge University Pressen
dc.rights© International Astronomical Unionen
dc.subjectGravitational lensingen
dc.subject(Galaxy:) globular clusters: generalen
dc.titleDetection of IMBHs from microlensing in globular clustersen
Appears in Collections:IIAP Publications

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