  Optical and X-ray observations are presented here of a newly reported X-ray
transient system in the Small Magellanic Cloud. The data reveal many previously
unknown X-ray detections of this system and clear evidence for a 49.995d binary
period. In addition, the optical photometry show recurring outburst features at
the binary period which may well be indicative of the neutron star interacting
with a circumstellar disk around a Be star.
