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Detection of IMBHs from microlensing in globular clusters

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dc.contributor.author Safonova, M
dc.contributor.author Rahvar, S
dc.contributor.author Bond, I
dc.contributor.author Hearnshaw, J
dc.contributor.author Stalin, C. S
dc.date.accessioned 2009-08-04T10:09:55Z
dc.date.available 2009-08-04T10:09:55Z
dc.date.issued 2008-10
dc.identifier.citation Chakrabarti, Sandip K. and Majumdar, Archan S. eds., Observational evidence for black holes in the universe., Proceedings of the 2nd Kolkata Conference on Observational Evidence for Black Holes in the Universe held in Kolkata India, 10 - 15 February 2008 and the Satellite Meeting on Black Holes, Neutron stars, Gamma-Ray Bursts, and Gamma-Ray Bursts held 16 - 17 February, 2008, pp. 121 - 126 en
dc.identifier.isbn 978-0-7354-0582-0
dc.identifier.uri http://hdl.handle.net/2248/4705
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 (10/sup2-10/sup4 M/subsolar) black holes, just as galaxies do, stimulates the searches and the development of new methods for proving their existence. Most of the attempts in search of the central black holes (BHs) are indirect and present enormous observational difficulties due to the crowding of stars in the GCs cores. 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 American Institute of Physics en
dc.relation.ispartofseries AIP Conference Proceedings; Vol. 1053
dc.relation.uri http://adsabs.harvard.edu/abs/2008AIPC.1053..121S en
dc.relation.uri http://dx.doi.org/10.1063/1.3009470 en
dc.rights © American Institute of Physics en
dc.subject Globular Star Clusters en
dc.subject Gravitational Waves en
dc.subject Black Holes en
dc.subject Galaxies en
dc.title Detection of IMBHs from microlensing in globular clusters en
dc.type Article en


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