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The nature of gravitational waves in a generalized gravitation theory isinvestigated. The linearized field equations and the metric tensor quadrupolemoment power and the decrease in radius of an inspiralling binary system of twocompact objects are derived. The generalized Kerr metric describing a spinningblack hole is determined by its mass $M$ and the spin parameter $a=cS/GM^2$.The LIGO-Virgo collaboration data is fitted with smaller binary black holemasses in agreement with the current electromagnetic, observed X-ray binaryupper bound for a black hole mass, $M\lesssim 10M_\odot$.

LIGO GW150914 and GW151226 Gravitational Wave Detection and Generalized Gravitation Theory (MOG)