We review what has been learnt and what remains unknown about the physics of
hot enhancons following studies in supergravity. We recall a rather general
family of static, spherically symmetric, non-extremal enhancon solutions
describing D4 branes wrapped on K3 and discuss physical aspects of the
solutions. We embed these solutions in the six dimensional supergravity
describing Type IIA strings on K3 and generalize them to have arbitrary charge
vector. This allows us to demonstrate the equivalence with a known family of
hot fractional D0 brane solutions, to widen the class of solutions of this
second type and to carry much of the discussion across from the D4 brane
analysis. In particular we argue for the existence of a horizon branch for
these branes.Comment: 25 pages, Late