Me. Galavis et al., ATOMIC DATA FROM THE IRON PROJECT .10. EFFECTIVE COLLISION STRENGTHS FOR INFRARED TRANSITIONS IN SILICON-LIKE AND SULFUR-LIKE IONS, Astronomy & Astrophysics. Supplement series, 111(2), 1995, pp. 347-357
Effective collision strengths for the electron impact excitation of tr
ansitions within the 3s(2)3p(q) ground configuration of ions in the si
licon (q = 2) and sulphur (q = 4) isoelectronic sequences are presente
d. We consider here astrophysically abundant ions that give rise to in
frared transitions within their P-3(J) ground term, namely, S III, Cl
IV, Ar V, K VI, Ca VII, Ar III, K IV and Ca V. The configuration-inter
action target approximations developed for the R-matrix calculations i
nclude single and double excitations within the n = 3 complex. An atte
mpt is made to include a sufficient number of n = 3 target states in t
he close-coupling expansion so as to account for the prominent resonan
ce effects that dominate the energy regions of interest, but developme
nt is handicapped since the energies of many of these states have not
been measured. The contributions from resonances converging to n = 4 t
arget states, which begin to appear in the energy region of interest f
or the lower members of the sequence, are studied in the case of S III
. Relativistic effects in the target, which become important for high
Z, are examined in Ca V. Both of these contributions to the excitation
cross sections are found to be relatively small (< 20%) and therefore
are neglected in the other systems under consideration. The good agre
ement found with previous calculations for S III and Ar III suggests t
hat the present collisional data for the weakly ionised members of the
sequence may be accurate to within 20%, but we expect this rating to
deteriorate for higher Z due to the neglect of extra contributing thre
sholds.