  PSR J2032+4127 has recently been identified as being in a long period (45-50
years) binary in a highly eccentric orbit with the Be star MT91 213. Periastron
is due to occur in November 2017 and this rare occurrence has prompted a
multiwavelength monitoring campaign to determine if the system is a gamma-ray
binary, and, if so, to study what would be only the second gamma-ray binary
with a known compact object. In the same direction as TeV J2032+4130, gamma-ray
emission from this binary system could be related to the extended very high
energy gamma-ray emission from that region. As part of this monitoring,
observations are being conducted by Swift, Fermi-LAT and VERITAS. We present
the status of those observations, preliminary results and the plan for
continued monitoring through periastron.
