Abstract
We developed a method that allows us to estimate the high energy gamma ray luminosity of intermediate mass black holes (IMBH) located in the central regions of globular clusters. Our calculations are based on the relation between the relativistic jet kinetic power and the luminosity of the gamma ray radiation that is produced by the jet itself. The power of a relativistic jet is determined via the Blandford–Znajek mechanism. Our calculations show that the contribution of the central IMBH in gamma ray luminosity is comparable with the contribution of the population of millisecond pulsars.
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