  We study Hawking radiation from three-dimensional black holes. For this
purpose the emission of charged scalar and charged fermionic particles is
investigated from charged BTZ black holes, with and without rotation. We use
the quantum tunneling approach incorporating WKB approximation and spacetime
symmetries. Another class of black hole which is asymptotic to a Sol
three-manifold has also been investigated. This procedure gives us the
tunneling probability of outgoing particles, and we compute the temperature of
the radiation for these black holes. We also consider the quantum tunneling of
particles from black hole asymptotic to Sol geometry.
