  MAGIC is one of the main instruments for exploring the galactic gamma-ray sky
from ground in the energy range of 50 GeV - 50 TeV. It consists of two 17 m
diameter imaging atmospheric Cherenkov telescopes located at the Roque de los
Muchachos Observatory, on the Canary island of La Palma. Thanks to its
excellent sensitivity, MAGIC has conducted relevant studies on galactic objects
of different types at Very High Energies. Among them, the Crab pulsar up to TeV
energies, the spectral cut-off of the supernova remnant Cassiopeia A, the
super-orbital variability of the binary system LSI +61 303, the search for
microqusars, multi-year observations of the Galactic Center and follow-up
studies of unidentified HAWC sources. In many cases, the results from these
observations challenge our understanding of the underlying emission mechanisms.
Here we review the latest results from the observation of these galactic
sources with MAGIC.
