  We report the discovery of two hot-Jupiter planets, each orbiting one of the
stars of a wide binary system. WASP-94A (2MASS 20550794-3408079) is an F8 type
star hosting a transiting planet with a radius of 1.72 +/- 0.06 R_Jup, a mass
of 0.452 +/- 0.034 M_Jup, and an orbital period of 3.95 days. The
Rossiter-McLaughlin effect is clearly detected, and the measured projected
spin-orbit angle indicates that the planet occupies a retrograde orbit.
WASP-94B (2MASS 20550915-3408078) is an F9 stellar companion at an angular
separation of 15" (projected separation 2700 au), hosting a gas giant with a
minimum mass of 0.618 +/- 0.028 M_Jup with a period of 2.008 days, detected by
Doppler measurements. The orbital planes of the two planets are inclined
relative to each other, indicating that at least one of them is inclined
relative to the plane of the stellar binary. These hot Jupiters in a binary
system bring new insights into the formation of close-in giant planets and the
role of stellar multiplicity.
