  We study the production of Hot Jupiters (HJs) in stellar binaries. We show
that the "eccentric Kozai-Lidov" (EKL) mechanism can play a key role in the
dynamical evolution of a star-planet-star triple system. We run a large set of
Monte Carlo simulations including the secular evolution of the orbits, general
relativistic precession, and tides, and we determine the semi-major axis,
eccentricity, inclination and spin-orbit angle distributions of the HJs that
are produced. We explore the effect of different tidal friction parameters on
the results. We find that the efficiency of forming HJs when taking the EKL
mechanism into account is higher then previously estimated. Accounting for the
frequency of stellar binaries, we find that this production mechanism can
account for about 30% of the observed HJ population. Current observations of
spin-orbit angles are consistent with this mechanism producing \sim 30% of all
HJs, and up to 100% of the misaligned systems. Based on the properties of
binaries without a HJ in our simulations, we predict the existence of many
Jupiter-like planets with moderately eccentric and inclined orbits and
semi-major axes of several AU.
