  Analysis of the surface composition of the suspected cool RV Tauri star CE
Vir shows no systematic trend in depletions of elements with respect to
condensation temperature. However, there is a significant depletion of the
elements with respect to the first ionization potential of the element. The
derived Li abundance of log $\epsilon$ (Li) = 1.5$\pm$0.2 indicates production
of Li in the star. Near infrared colours indicate sporadic dust formation close
to the photosphere.
