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A binary system of identical corotating Kerr sources is studied afterderiving the corresponding 3-parametric asymptotically flat exact solution.Both sources are apart from each other by means of a massless strut (conicalsingularity). In the context of black holes, the analytical functional form ofeach horizon {\sigma} is expressed in terms of arbitrary Komar physicalparameters: mass M, angular momentum J (with parallel spin), and the coordinatedistance R between the center of each horizon. Later on, all thethermodynamical properties related to the horizon are depicted by conciseformulae. Finally, the extreme limit case is obtained as a 2-parametricsubclass of Kinnersley-Chitre metric.

Corotating two-body system of identical Kerr sources