  We obtain a newly charged BBMB (Bocharova-Bronnikov-Melnikov-Bekenstein)
black hole solution from the Einstein-Weyl-Maxwell-conformal (conformally
coupled) scalar theory with a positive Weyl coupling parameter $m^2_2$
numerically. This solution has a primary scalar hair, compared to a secondary
scalar hair in the charged BBMB black hole solution. The limiting case of
$m_2^2\to\infty$ leads to the series form of the charged BBMB black hole
solution. However, for $m^2_2<0$, we could not obtain any asymptotically flat
black hole solution with scalar hair.
