STARK-BROADENING DATA FOR STELLAR PLASMA RESEARCH

Results of an effort to provide to astrophysicists and physicists a se t of Stark broadening parameters that is as complete as possible are p resented. Such parameters are needed for stellar opacity calculations, stellar atmosphere modelling, abundance determinations, and diagnosti cs of various plasmas in astrophysics, physics, and plasma technology. The Stark broadening was treated using a semiclassical perturbation a nd modified semiempirical approaches, keywords: lines-profile-atomic a nd molecular data-CP stars.