  Galactic cosmic rays reach energies of at least several PeV, and their
interactions should generate $\gamma$-rays and neutrinos from decay of
secondary pions. Therefore, Galactic sources have a guaranteed contribution to
the total high-energy cosmic neutrino flux observed by IceCube. Assuming that
the highest energy $\gamma$-rays are pionic, promising neutrino source
candidates have been identified based on their spectra, and observing them is
likely over the lifetime of the IceCube experiment. Here, we present the search
for Galactic sources of high-energy cosmic neutrinos by focusing on sources
identified by HAWC's very high energy $\gamma$-ray survey.
