We present subarcsecond optical imaging and polarization observations of fi
ve optical hot spot candidates in the classical double radio sources 3C 111
, 3C 303, 3C 351, 3C 390.3, and PKS 2135-147. On the basis of positional co
incidence, optical appearance, and polarization, all four 3C sources appear
to have genuine optical counterparts to radio hot spots, whereas in PKS 21
35-147 the hot spot candidate turns out to be an unrelated field galaxy. We
also confirm the first ever optical double hot spot in the source 3C 351.