  We present high spatial resolution images that demonstrate the hot Jupiters
WASP-12b and HAT-P-8b orbit the primary star of hierarchical triple star
systems. In each case, two distant companions with colors and brightness
consistent with M dwarfs co-orbit the planet host as well as one another. Our
adaptive optics images spatially resolve the secondary around WASP-12,
previously identified by Bergfors et al. 2011 and Crossfield et al. 2012, into
two distinct sources separated by 84.3+/-0.6 mas (21 +/- 3 AU). We find that
the secondary to HAT-P-8, also identified by Bergfors et al. 2011, is in fact
composed of two stars separated by 65.3+/-0.5 mas (15+/-1 AU). Our follow-up
observations demonstrate physical association through common proper-motion.
HAT-P-8 C has a particularly low mass, which we estimate to be 0.18+/-0.02Msun
using photometry. Due to their hierarchy, WASP-12 BC and HAT-P-8 BC will enable
the first dynamical mass determination for hot Jupiter stellar companions.
These previously well-studied planet hosts now represent higher-order
multi-star systems with potentially complex dynamics, underscoring the
importance of diffraction-limited imaging and providing additional context for
understanding the migrant population of transiting hot Jupiters.
