Astron. Astrophys. Suppl. Ser.
Volume 123, Number 1, May II 1997
|Page(s)||147 - 158|
|Published online||15 May 1997|
Orthogonal operator calculation of E1, M1 and E2 transition probabilities in Ti III and V IV
Van der Waals-Zeeman Instituut, Universiteit van Amsterdam, Valckenierstraat 65-67, 1018 XE Amsterdam, The Netherlands
Send offprint request to: A.J.J. Raassen
Accepted: 13 September 1996
Transition probabilities in the iron group spectra Ti III and V IV are obtained from an accurate description of the 8 lowest even and 4 lowest odd configurations of the atomic system. Results are compared with experiment and current databases.
Key words: atomic data / Sun: photosphere / stars: abundances
© European Southern Observatory (ESO), 1997