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In this paper we determined values of a spin of central black holes of theintermediate masses in globular clusters. For determination of value of a spinwe used the known relation between the kinetic power of the relativistic jetand observable radio-luminosity of the region near to a central black hole, andour estimates have based on the known Blandford-Znajek mechanism. The value ofa magnetic field strength near the event horizon of a black hole was derivedvia magnetic coupling mechanism. Accretion rate was derived using Bondi-Hoylemechanism.

Black holes of intermediate masses in globular clusters: constraints on a spin of a black hole