Wavelengths and transition rates are given for E1 transitions between singlet3S,3P,3D, and1F states, between triplet3S,3P, and3D states, and between triplet3P1and singlet1S0states in ions of astrophysical interest: helium-like carbon, nitrogen, oxygen, neon, silicon, and argon. All possible El transitions between states with J ≤ 3 and n ≤ 6 are considered. Energy levels and wave functions used in calculations of the transition rates are obtained from relativistic configuration-interaction calculations that include both Coulomb and Breit interactions.
CITATION STYLE
Johnson, W. R., Savukov, I. M., Safronova, U. I., & Dalgarno, A. (2002). E1 Transitions between States with n = 1–6 in Helium‐like Carbon, Nitrogen, Oxygen, Neon, Silicon, and Argon. The Astrophysical Journal Supplement Series, 141(2), 543–557. https://doi.org/10.1086/340547
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