  We revisit the shadow of rotating traversable wormholes discussing the role
of the wormhole throat in the shadow formation. For certain classes of
wormholes the throat serves as a potential barrier for light rays with
particular impact parameters, thus modifying the shadow shape. We consider a
couple of wormhole solutions and examine the structure of their shadow images,
and the intrinsic mechanisms for their formation. Some of the shadows possess
cuspy edges, which arise due to the interplay of two distinct families of
unstable spherical orbits. These solutions provide examples, in which the
explicit mechanism for cusp formation can be uncovered.
