We resolved the brightest stars in 5 nearby blue compact dwarf galaxies wit
h NICMOS aboard HST in J and H. In all galaxies, RGB stars were detected. T
his finding allows an improved estimate of the distances of these galaxies
and sets a lower limit to the age of the old stellar component of 1 Gyr. Fu
rther, we detected a pronounced AGB population, including - in all but one
- also TP-AGB stars. Our data do not support the hypothesis that very low m
etallicity BCD galaxies may have formed their first stars only recently.