Detection of IMBHs from microlensing in globular clusters

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5709

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DC Field	Value	Language
dc.contributor.author	Safonova, M	-
dc.contributor.author	Rahvar, S	-
dc.date.accessioned	2012-02-28T16:12:53Z	-
dc.date.available	2012-02-28T16:12:53Z	-
dc.date.issued	2007-04	-
dc.identifier.citation	International Astronomical Union Symposium; No. 238, pp. 439-440	en
dc.identifier.uri	http://hdl.handle.net/2248/5709	-
dc.description.abstract	Globular 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.iso	en	en
dc.publisher	Cambridge University Press	en
dc.relation.uri	http://dx.doi.org/10.1017/S1743921307005844	en
dc.rights	© International Astronomical Union	en
dc.subject	Gravitational lensing	en
dc.subject	(Galaxy:) globular clusters: general	en
dc.title	Detection of IMBHs from microlensing in globular clusters	en
dc.type	Article	en
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