  We have identified 85 regions of enhanced H-Alpha emission at |b| > 10
degrees subtending approximately 1 degree or less on the Wisconsin H-Alpha
Mapper (WHAM) sky survey. These high latitude ``WHAM point sources'' have
H-Alpha fluxes of 10^{-11} to 10^{-9} erg cm^-2 s^-1, radial velocities within
about 70 km/s of the LSR, and line widths that range from less than 20 km/s to
about 80 km/s (FWHM). Twenty nine of these enhancements are not identified with
either cataloged nebulae or hot stars and appear to have kinematic properties
that differ from those observed for planetary nebulae. Another 14 enhancements
are near hot evolved low mass stars that had no previously reported detections
of associated nebulosity. The remainder of the enhancements are cataloged
planetary nebulae and small, high latitude H II regions surrounding massive O
and early B stars.
