A&A Supplement series, Vol. 122, May II 1997, 147-158
Received June 21; accepted September 13, 1996
A.J.J. Raassen - P.H.M. Uylings
Send offprint request: A.J.J. Raassen
Van der Waals-Zeeman Instituut, Universiteit van Amsterdam, Valckenierstraat 65-67, 1018 XE Amsterdam, The Netherlands
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.
keywords: atomic data -- Sun: photosphere -- stars: abundances