Supernova remnants interacting with molecular clouds as seen with
  H.E.S.S
  About 30 Galactic supernova remnants (SNRs) are thought to be physically
associated with molecular clouds (MCs). These systems are prime \g-ray source
candidates as the accelerated particles from shock fronts collide with the
surrounding high-density medium thus emitting gamma-rays through hadronic
interactions. However only a handful of such interacting SNRs are detected at
TeV energies. We report the current status of the High Energy Stereoscopic
System (H.E.S.S.) observations towards these SNR-MC systems, with a particular
emphasis on the latest results.
