  The recent results from ground based $\gamma$-ray detectors (HESS, MAGIC,
VERITAS) provide a population of TeV galactic $\gamma$-ray sources which are
potential 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 vice
versa; the detectability of $\nu$ flux implies a minimum flux of the
accompanying $\gamma$-rays (assuming the internal and the external absorption
of $\gamma$-rays is negligible). Using this minimum flux, it is possible to
find the sources which can be detected with cubic-kilometer telescopes. I will
discuss the possibility to detect HE neutrinos from powerful galactic
accelerators, 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 be
detected by current generation of instruments (IceCube and Km3Net). It will be
shown 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 discussed
during recent gamma-ray activity, showing that in the future such kind of
activities could produce detectable flux of HE $\nu$-s
