  X-ray and gamma-ray binaries are systems consisting of a compact object and
normally a non-degenerate companion star. Most of these sources have been shown
to emit radiation in a broad frequency range, from radio up to X-rays and
sometimes gamma rays. We report on recent results in very high-energy gamma
rays above 100 GeV obtained by the MAGIC Collaboration for the Galactic X-ray
binaries MAXI J1820+070 and 1A 0535+262, and the gamma-ray binary HESS
J0632+057. Multiwavelength data at lower energies are also provided for a
better contextualisation of the sources.
