  Thermodynamics of a large family of black holes from electrovacuum solutions
of Einstein's equations is studied. This family includes rotating and
non-accelerating black holes with NUT charge, and rotating and accelerating
black holes. The surface gravity, Hawking temperature and the area laws for
these black holes are presented. The first law of thermodynamics is also given.
An interesting outcome of our analysis is the restriction obtained on the
magnitude of acceleration for these black holes.
