  We present the preliminary results of an ongoing series of spectroscopic
observations of the Small Magellanic Cloud star LHA 115-S 18 (S18), which has
demonstrated extreme photospheric and spectroscopic variability that, in some
respects, is reminiscent of Luminous Blue Variables (LBVs). In contrast to our
previously published results, between 2012-2015 S18 remained in an spectral
state intermediate between S18's "hot" and "cool" extremes. In conjunction with
contemporaneous OGLE-IV photometric monitoring of S18, these data will be used
to determine the characteristic timescale of the variability and search for
periodicities, in particular binary modulated periodicity. We also present the
results of a pilot study of the LMC star LHA 120-S 134.
