  VERITAS (Very Energetic Radiation Imaging Telescope Array System) is one of
the most sensitive currently operating arrays of imaging atmospheric Cherenkov
telescopes, which detect very high-energy (VHE; E > 100 GeV) gamma rays.
VERITAS is currently in its 11th year of full-array operations with four
12m-diameter telescopes. Many Galactic sources of VHE gamma rays have been
detected by VERITAS, such as pulsar wind nebulae, binary systems, and supernova
remnants, and the study of VHE emission from these objects has enabled a deeper
understanding of the underlying physical processes responsible for the observed
gamma rays. Recent highlights from the VERITAS Galactic science program will be
presented, including results on pulsar searches, follow-up of sources detected
by HAWC, and the 50-year-period binary PSR J2032+4127.
