Atomic-data for resonance absorption lines. II. Wavelengths longward of the lyman limit for heavy elements

This compilation extends the 1991 listing of atomic data by Morton to the h eavier stable elements from germanium to bismuth. Technetium, thorium, and uranium are added because they can live long enough to be astrophysically d etectable. The tabulation emphasizes resonance lines, i.e., lines the lower level of which is the ground state, or an excited fine-structure state of the ground term, and is restricted to wavelengths longward of the H I Lyman limit at 911.75 Angstrom. This paper has attempted to review all data publ ished by mid-1999 and includes some later material. The tables contain the best data available to the author on level designati ons, ionization potentials, vacuum and air wavelengths, lower and upper ene rgy levels, statistical weights, transition probabilities, natural damping constants (reciprocal lifetimes), oscillator strengths, and the often-used combinations of log gf and log lambdaf: All ion stages with classified line s are included. Individual components resulting from isotope shift and hype rfine structure are listed explicitly for Rb I, Cs I, Hg I and Hg II, Ti II , and Pb II. The accompanying text provides references, explanations for th e critical selection of data, and notes indicating where new measurements o r calculations are needed. This compilation should be particularly useful in the analysis of interstel lar and quasar absorption lines and other astrophysical sites where the den sity of particles and radiation is low enough to excite only the lowest ato mic levels. The data also are relevant to the study of stellar atmospheres, particularly those with enhanced abundances of heavy elements.