  We have obtained HST NICMOS snapshot images of ten BALQSOs and four
radio-quiet non-BALQSOs to search for extended narrow-line regions. For each
object we obtained an image in the F160W filter and a narrow-band image in
either H-alpha, H-beta, or [O ii]. We find no detections of extended
narrow-line emission in the sample. We generate simulated images of QSOs with
extended narrow-line regions to place limits on the amount of flux that may be
present, and we conclude that BALQSOs cannot be more than several times
brighter in extended emission than typical type 2 AGN. Spatially unresolved
H-alpha emission is detected in all nine objects observed in this line, which
we attribute to broad H-alpha emission. The five detected BALQSOs have derived
H-alpha equivalent widths that are larger than those of the four non-BALQSOs by
a factor of around 2 on average. This may point to an intrinsic difference
between the rest-frame optical spectral properties of BALQSOs and non-BALQSOs.
