Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apjs...73..555o&link_type=abstract
Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 73, July 1990, p. 555-602. Research supported by the Dynamic Expl
Astronomy and Astrophysics
Astrophysics
22
Energy Levels, Hydrogen Atoms, Oscillator Strengths, Rydberg Series, Transition Probabilities, Electron Energy, Radiative Recombination, Recombination Coefficient
Scientific paper
Results are presented from calculations of the optical oscillator strength f(n, l, n-squared epsilon), for hydrogenic atoms in the initial state n., and the final energy state, epsilon, for the range n between 1 and 50, l between 0 and 26, and epsilon between 0 and 10 to the 7th rydbergs/n-squared. In addition, the bound-continuum oscillator strength is tabulated. The results of the calculations are compared with previously published values, showing satisfactory agreement.
Guimaraes Patricia T.
Omidvar Kazem
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