  We present new follow-up observations of two ultra-diffuse galaxies (UDGs),
part of a total sample of five chosen for their distorted morphologies,
suggestive of tidal influence. Using Hubble Space Telescope Advanced Camera for
Surveys F555W and F814W imaging, we identify 8+/-2 globular clusters (GCs) in
KUG 0203-Dw1 and 6+/-2 in KDG 013, abundances that are fairly typical for
normal dwarf galaxies of similar stellar mass. Jansky Very Large Array data
reveal a clear HI detection of KUG 0203-Dw1 with a gas mass estimate of
log(MHI/Msun) < 7.4 and evidence of active stripping by the host. HI gas is
found near the location of KDG~013 but is likely unrelated to the UDG itself
due to the morphology and the numerous gas tails within the host group. Given
that these UDGs have GC abundances typical for galaxies at their luminosity,
these findings suggest that they likely originated as normal dwarf galaxies
that have been subjected to significant stripping and tidal heating, causing
them to become more diffuse. These two UDGs complete a sample of five
exhibiting tidal features in the Canada-France-Hawaii Telescope Legacy Survey
area (CFHTLS; ~150 sq deg), including UDGs with and without UV emission,
indicative of recent star formation. Four UDGs in this sample, consistent with
dwarfs `puffed-up' by tidal interactions, contrast with an outlier, suggesting
a dwarf merger origin. These findings indicate that tidal heating of dwarfs is
a viable formation pathway for UDGs.
