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The recent results from ground based $\gamma$-ray detectors (HESS, MAGIC,VERITAS) provide a population of TeV galactic $\gamma$-ray sources which arepotential sources of High Energy (HE) neutrinos. Since the $\gamma$-rays and$\nu$ -s are produced from decays of neutral and charged pions, the flux of TeV$\gamma$-rays can be used to estimate the upper limit of $\nu$ flux and viceversa; the detectability of $\nu$ flux implies a minimum flux of theaccompanying $\gamma$-rays (assuming the internal and the external absorptionof $\gamma$-rays is negligible). Using this minimum flux, it is possible tofind the sources which can be detected with cubic-kilometer telescopes. I willdiscuss the possibility to detect HE neutrinos from powerful galacticaccelerators, such as Supernova Remnants (SNRs) and Pulsar Wind Nebulae (PWNe)and show that likely only RX J1713.7-3946 , RX J0852.0-4622 and Vela X can bedetected by current generation of instruments (IceCube and Km3Net). It will beshown also, that galactic binary systems could be promising sources of HE $\nu$-s. In particular, $\nu$-s and $\gamma$-rays from Cygnus X-3 will be discussedduring recent gamma-ray activity, showing that in the future such kind ofactivities could produce detectable flux of HE $\nu$-s

Galactic sources of high energy neutrinos: Expectation from gamma-ray data