Abstract
I am attempting to produce line lists for all atoms and diatomic molecules that are important in stars. I collect all published data on spectrum analysis and oscillator strengths. I compute the energy levels, wavelengths, gf values, and damping constants that are not available from the literature. Line lists have been computed for diatomic molecules H2, CII, NH, OH, MgH, SiH, CN, C2, CO, SiO, and TiO, and for the iron group atoms Ca 1-IX to Ni 1-IX. These lists total 58 million lines. These calculations are being revised as new laboratory data become available. The work is being extended to other diatomic molecules, to lighter and heavier elements, and to higher stages of ionization. Key words: ATOMIC PROCESSES - MOLECULAR PROCESSES - TRANSITION PROBABILITIES
