Multipolar expansion profile of Hawking radiation on Kerr black holes I would be very curious if Kerr black holes emit Hawking radiation at the same temperature in the equatorial bulges and in their polar regions. I've been looking some reference for this for a couple of months now but i haven't been successful yet.
According to this answer, Too great Hawking radiation could thwart mass from being feed into a black hole, so this begs the question: Could possibly a (very small) Kerr black hole be able to accept infalling matter if it falls along the rotational axis? Possibly, since 4D Kerr black holes angular momentum are bounded by extremality condition, the possible difference in temperature between polar and equatorial regions will not be wide enough to be interesting (possibly not bigger than an order of magnitude), but it would still be interesting to know how much is the temperature ratio. It could very well be zero, or more intriguingly, could depend on the black hole mass. But in any case, i doubt that the ergosphere region will not interact nontrivially to boost equatorial Hawking radiation to some degree
Thoughts?
 A: I don't have a full answer to your question, but your question did make me realize that the Hawking radiation must be carrying away angular momentum from a rotating Kerr black hole. If it only carried away energy (mass) the Kerr black hole would become extremal as it lost mass but kept the same angular momentum. This, I think, proves that there has to be asymmetries in the Hawking radiation from a Kerr black hole. 
One way to carry away angular momentum would be for a higher flux or energy of Hawking radiation in the forward direction of rotation at the equator. I think this implies that limb coming towards you would look like it is at a higher temperature that the limb that is receding from your point of view.  Another way to carry away angular momentum would be to emit partially (circularly) polarized radiation from the polar regions but then these would not look like black body radiation. I don't know how to calculate the effects, but I would not be surprised if there was a temperature variation on the event horizon. But I could be wrong.
"lurscher" gave a link to an article that answers this question.  The abstract says:

Particle emission rates from a black hole. II. Massless particles from
  a rotating hole 
Don N. Page W. K. Kellogg Radiation Laboratory, California Institute
  of Technology, Pasadena, California 91125
The calculations of the first paper of this series (for nonrotating
  black holes) are extended to the emission rates of massless or nearly
  massless particles from a rotating hole and the consequent evolution
  of the hole. The power emitted increases as a function of the angular
  momentum of the hole, for a given mass, by factors of up to 13.35 for
  neutrinos, 107.5 for photons, and 26 380 for gravitons. Angular
  momentum is emitted several times faster than energy, so a rapidly
  rotating black hole spins down to a nearly nonrotating state before
  most of its mass has been given up. The third law of black-hole
  mechanics is proved for small perturbations of an uncharged hole,
  showing that it is impossible to spin up a hole to the extreme Kerr
  configuration. If a hole is rotating fast enough, its area and entropy
  initially increase with time (at an infinite rate for the extreme Kerr
  configuration) as heat flows into the hole from particle pairs created
  in the ergosphere. As the rotation decreases, the thermal emission
  becomes dominant, drawing heat out of the hole and decreasing its
  area. The lifetime of a black hole of a given mass varies with the
  initial rotation by a factor of only 2.0 to 2.7 (depending upon which
  particle species are emitted). If a nonrotating primordial black hole
  with initial mass 5 × 1014 g would have just decayed away within the
  present age of the universe, a hole created maximally rotating would
  have just died if its initial mass were about 7 × 1014 g. Primordial
  black holes created with larger masses would still exist today, but
  they would have a maximum rotation rate determined uniquely by the
  present mass. If they are small enough today to be emitting many
  hadrons, they are predicted to be very nearly nonrotating.

