  The H.E.S.S. Galactic Plane Survey has detected very-high-energy (VHE)
gamma-ray emission from 78 sources in the Milky Way. These sources belong to
different object classes (pulsar wind nebulae, supernova remnants or binary
systems) and some of these sources remain unidentified. The gamma-ray emission
of these objects may be of leptonic or hadronic origin and gamma-ray
observations alone cannot distinguish between these two scenarios. The
detection of neutrino emission would provide evidence for a hadronic scenario
in these objects.
  Based on the observed gamma-ray spectra we predict the neutrino emission of
these sources under the hypothesis that the emission is solely of hadronic
origin. This prediction relies entirely on observation and is independent of
the source class, the distance or the ambient target material. We use these
predictions to create an empirical model for the neutrino emission of the Milky
Way. This model can be used to search for neutrino emission from individual
gamma-ray sources as well as testing for neutrino emission from potential
source populations in the Milky Way.
