  Flare stars were discovered in the late 1940s in the solar vicinity and were
named UV Cet-type variables (classical FSs). Among the FSs within 100 pc we
search for young stars. For the search we take spectra with sufficient
resolution to resolve Lithium at 6707 \AA and Calcium at 6718 \AA of all the
stars. The real young stars are prime targets for the search of extra-solar
planets by direct imaging.
