  In order to complete Stark broadening data for Ne II, and O III lines, needed
for analysis of stellar atmospheres, we determined, within the semiclassical
perturbation method, the missing Stark broadening parameters for the broadening
by collisions with protons and ionized helium, for 15 Ne II and 5 O III
multiplets. Also, electron, proton, and ionized helium impact broadening
parameters for an important Ne II multiplet in the visible part of the
spectrum, and for three Ne III multiplets, were calculated. The obtained data
will be included in the STARK-B database, which is a part of Virtual Atomic and
Molecular Data Center.
