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Issue A&A
Volume 410, Number 1, October IV 2003
Page(s) 349 - 358
Section Celestial mechanics and astrometry
DOI http://dx.doi.org/10.1051/0004-6361:20031193



A&A 410, 349-358 (2003)
DOI: 10.1051/0004-6361:20031193

Effective collision strengths for transitions in Fe XV

K. M. Aggarwal1, F. P. Keenan1 and A. Z. Msezane2

1  Department of Pure and Applied Physics, The Queen's University of Belfast, Belfast BT7 1NN, Northern Ireland, UK
2  Center for Theoretical Studies of Physical Systems, Clark Atlanta University, Atlanta Ga 30304, USA

(Received 10 June 2003 / Accepted 30 July 2003 )

Abstract
Collision strengths for transitions among the energetically lowest 53 fine-structure levels belonging to the (1s 22s 22p 6) 3 ${\ell}^2$, 3 ${\ell}$3 ${\ell}^{'}$, 3s4 ${\ell}$ and 3p4s configurations of Fe XV are computed, over an electron energy range below 160 Ryd, using the Dirac Atomic R-matrix Code (DARC) of Norrington & Grant (2003). Effective collision strengths, obtained after integrating the collision strengths over a Maxwellian distribution of electron energies, have also been calculated. These results of effective collision strengths are tabulated for all 1378 inelastic transitions over a wide temperature range of 10 5 to 10 7 K. Comparisons are also made with other R-matrix calculations and the accuracy of the results is assessed.


Key words: atomic data -- atomic processes

Offprint request: K. M. Aggarwal, K.Aggarwal@qub.ac.uk


Tables at the CDS



© ESO 2003

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