  A static spherically symmetric black hole usually turns out to be either a
Schwarzschild black hole or a Reissner-Nordstr\"{o}m black hole. This result
was summarised by Ruffini and Wheeler as the so-called no hair conjecture which
states that for a spherically symmetric black hole only the information about
mass ($M$) and electric charge ($e$) of the black hole is available for an
external observer. In this work, we calculate the emission rate of charged
particles from an asymptotically flat charged spherically symmetric black hole
endowed with a scalar hair using a semi-classical tunneling formalism. We
observe that the total entropy of the black hole contains an energy-dependent
part due to the scalar charge. The upper bound on the charge-mass ratio of the
emitted particles is also observed to decrease with the scalar charge as well.
