Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26as...84..563a&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 84, no. 3, Sept. 1990, p. 563-600. Research supported by SNS
Astronomy and Astrophysics
Astrophysics
43
Beryllium, Carbon, Isoelectronic Sequence, Nitrogen Ions, Oscillator Strengths, Oxygen Ions, Atomic Structure, Stellar Envelopes, Stellar Evolution, Stellar Structure
Scientific paper
Oscillator strengths for the observed lines of C III, N IV, and O V are compiled. All the data published between 1966 and 1989 are reported and critically analyzed. Recent exhaustive results of the OPACITY project are included. The level lifetimes measured for these ions are also compiled and compared to the theoretical lifetimes. Adopted gf-values are proposed from a weighted mean of the best theoretical results. These data concern 204, 190, and 140 multiplets of C III, N IV, and O V respectively, with an accuracy in the 10 percent range in most cases.
Allard Nicole
Artru Marie-Christine
Lanz Thierry
Le Dourneuf M.
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