Using Hipparcos parallaxes, we show that the metallic A-F giants found by
Hauck (1986) on the basis of their high Delta m_2 index in Geneva photometry
are on average more evolved than their non-metallic counterparts. Their mass
distribution, rate of binaries and vsini are shown to be incompatible with
those of Am stars, so that they cannot be descendants of the latter. They might
be former normal stars going through a short metal-rich phase at the very end
of their life on the Main Sequence.Comment: 3 pages, 1 figure, to appear in: Proc. of the 26th workshop of the
European Working Group on CP stars, eds. P. North, A. Schnell and J.
Ziznovsky, Contrib. Astr. Obs. Skalnate Pleso Vol. 27, No
