  We overview high-energy neutrinos from galactic sources, transparent to their
gamma-ray emission. We focus on young supernova remnants and in particular on
RX J1713.7-3946, discussing expectations and upper bounds. We also consider the
possibility to detect neutrinos from other strong galactic gamma-ray sources as
Vela Junior, the Cygnus Region and the recently discovered Fermi Bubbles. We
quantify the impact of the recent hint for a large value of $\theta_{13}$ on
high-energy neutrino oscillations.
