Computer Science
Scientific paper
Aug 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aipc..168...59p&link_type=abstract
AIP Conference Proceedings, Volume 168, pp. 59-70 (1988).
Computer Science
1
Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation, Oscillator Strengths, Lifetimes, Transition Moments, Plasma Diagnostic Techniques And Instrumentation, Atomic, Molecular, Ion, And Heavy-Particle Collisions
Scientific paper
With the primary aim of calculating stellar envelope opacities, a joint international collaboration is under way for the calculation of basic atomic data for radiative processes: oscillator strengths, photoionization cross sections, energy levels, radiative damping constants (including line broadening). Atomic calculations have been completed for the first ten isoelectronic sequences, H-like to Ne-like, going up to iron, and work is in progress on the third and fourth row atoms and isosequences. The close-coupling approximation is employed throughout using a new version of the R-matrix method. Particular emphasis is placed on the detailed resolution of the autoionization structures in the bound-free continuum.
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