Recent results of fits to comprehensive sets of K-, Sigma(-) and (p) o
ver bar atom data in terms of density-dependent optical potentials are
described and discussed. The introduction of density dependence impro
ves significantly the fit to the data in K- and Sigma(-) atoms and lea
ds to some novel results. For K- atoms, a substantial attraction of or
der 200 MeV at nuclear matter densities is predicted, with interesting
repercussions on (K) over bar condensation and on the evolution of st
rangeness in high-density stars. For Sigma(-) atoms the fitted potenti
al, which is attractive outside the nuclear surface, becomes repulsive
on the nuclear surface and inside, indicating that Sigma hyperons, ge
nerally, do not bind in nuclei. For (p) over bar atoms it is found tha
t a reasonable p-wave strength can be accommodated into the fitted opt
ical potential.