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The greybody factor and the Hawking temperature for a class of asymptoticallyflat charged dilatonic black holes are computed by using the low-energydynamics of scalar fields in the black hole background. In the semi-classicalapproximation, the Hawking temperature has a good agreement with the onecomputed from the surface gravity, which is independent of the magnetic (orelectric) charges of dilatonic black holes.

Greybody Factor and Hawking Radiation of Charged Dilatonic Black Holes