  We study the Hawking radiation (HR) of scalar and Dirac particles (fermions)
emitted from a rotating scalar hair black hole (RSHBH) within the context of
three dimensional ($3D$) Einstein gravity using non-minimally coupled scalar
field theory. Amalgamating the quantum tunneling approach with the
Wentzel--Kramers--Brillouin (WKB) approximation, we obtain the tunneling rates
of the outgoing particles across the event horizon. Inserting the resultant
tunneling rates into the Boltzmann formula, we then obtain the Hawking
temperature ($T_{H}$) of the $3D$ RSHBH.
