The detection of O vm emission lines in ultraviolet and optical spectr
a of high-excitation planetary-nebula central stars suggests an ''O VI
II sequence'' for these objects. Emission lines of O VII are also dete
cted. Seven out of ten central stars for these planetaries are known t
o be nonradial g-mode pulsators. The stars form a narrow strip when pl
otted on the log L/L(.)-log T-eff H-R diagram.