Free access
Issue
Astron. Astrophys. Suppl. Ser.
Volume 123, Number 1, May_II 1997
Page(s) 147 - 158
DOI http://dx.doi.org/10.1051/aas:1997309
DOI: 10.1051/aas:1997309

A&A Supplement series, Vol. 123, May II 1997, 147-158

Received June 21; accepted September 13, 1996

Orthogonal operator calculation of E1, M1 and E2 transition probabilities in Ti III and V IV

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

Abstract:

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


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