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In this review we shall comment on a few recent findings which strengthen theview that the black hole accretion has substantial amount of sub-Kepleriancomponent. The manifestation of this component is many fold. We discuss some ofthem. A general outline of the complex structure that emerges from themultitude of observations is presented. A detailed outline of what might begoing on in outburst sources is also discussed. The relationship amount thespectral and timing properties can be best understood by this picture. We claimthat the sub-Keplerian advective disk paradigm is a complete package. Sincesignatures of sub-Keplerian motion is already increasing in the literature, thewhole package must be correct.

Black Hole Accretion: From Quasars to Nano-Quasars