Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26as..131..499g&link_type=abstract
Astronomy and Astrophysics Supplement, v.131, p.499-522
Astronomy and Astrophysics
Astrophysics
46
Atomic Data, Atomic Processes
Scientific paper
As part of the IRON Project, radiative rates have been calculated for the E1, E2 and M1 transitions within the n=2 complex in ions of the boron isoelectronic sequence (6<= Z<= 28). The computations have been carried out with the atomic structure code superstructure which facilitates the generation of extended radiative datasets including configuration interaction, Breit-Pauli relativistic contributions and semi-empirical term-energy corrections. By means of extensive comparisons with the available datasets for this sequence, with detailed single-ion calculations and recent experiments, we have been able to assign accuracy ratings to the present A-values. We find that in general the spin-allowed and spin-forbidden E1 transitions are accurate to 10% and 20%, respectively, except for a few transitions in ions with Z<= 7 that are perturbed by admixture with low-lying n=3 states (e.g. 2ssp23l ) and for those affected by the avoided crossing of the 2s2psp2 \ sp2 S_{1/2} and sp2 P_{1/2} which takes place at Z ~ 22. It is concluded that, statistically, the present dataset is the most accurate to date for this astrophysically relevant sequence. A detailed table of the present transition probabilities is available in electronic form from the CDS via anonymous ftp 130.79.128.5
Galavis M. E.
Mendoza Carolina
Zeippen Claude J.
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