Free Access
| Issue |
Astron. Astrophys. Suppl. Ser.
Volume 123, Number 1, May II 1997
|
|
|---|---|---|
| Page(s) | 147 - 158 | |
| DOI | https://doi.org/10.1051/aas:1997309 | |
| Published online | 15 May 1997 | |
Astron. Astrophys. Suppl. Ser. 123, 147-158 (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
Received:
21
June
1996
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