Volume 543, July 2012
|Number of page(s)||9|
|Section||Atomic, molecular, and nuclear data|
|Published online||25 June 2012|
Atomic decay data for modeling K lines of iron peak and light odd-Z elements⋆
1 Astrophysique et Spectroscopie (ASPECT), Université de Mons – UMONS, 20 place du Parc, 7000 Mons, Belgium
2 IPNAS, Université de Liège, Campus du Sart Tilman, Bât. B15, 4000 Liège, Belgium
3 Centro de Física, Instituto Venezolano de Investigaciones Científicas (IVIC), PO Box 20632, Caracas 1020A, Venezuela
4 Department of Physics, Western Michigan University, Kalamazoo, MI 49008, USA
5 Department of Astronomy, University of Maryland, College Park, MD 20742, USA
6 NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
e-mail: email@example.com; firstname.lastname@example.org
Received: 18 April 2012
Accepted: 20 May 2012
Complete data sets of level energies, transition wavelengths, A-values, radiative and Auger widths and fluorescence yields for K-vacancy levels of the F, Na, P, Cl, K, Sc, Ti, V, Cr, Mn, Co, Cu and Zn isonuclear sequences have been computed by a Hartree-Fock method that includes relativistic corrections as implemented in Cowan’s atomic structure computer suite. The atomic parameters for more than 3 million fine-structure K lines have been determined. Ions with electron number N > 9 are treated for the first time, and detailed comparisons with available measurements and theoretical data for ions with N ≤ 9 are carried out in order to estimate reliable accuracy ratings.
Key words: atomic data / atomic processes / line: formation / X-rays: general
Full Tables 9 and 10 are available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (22.214.171.124) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/543/A44
© ESO, 2012
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