Line ratios for helium-like ions: Applications to collision-dominated plasmas

The line ratios R and G of the three main lines of He-like ions (triplet: r esonance, intercombination, forbidden lines) are calculated for C V, N VI, O VII, Ne IX, Mg XI, and Si XIII. These ratios can be used to derive electr on density ne and temperature T-e of hot late-type stellar coronae and O, B stars from high-resolution spectra obtained with Chandra (LETGS, HETGS) an d XMM-Newton (RGS). All excitation and radiative processes between the leve ls and the effect of upper-level cascades from collisional electronic excit ation and from dielectronic and radiative recombination have been considere d. When possible the best experimental values for radiative transition prob abilities are used. For the higher-Z ions (i.e. Ne IX, Mg XI, Si XIII) poss ible contributions from blended dielectronic satellite lines to each line o f the triplets were included in the calculations of the line ratios R and G for four specific spectral resolutions: RGS, LETGS, HETGS-MEG, HETGS-HEG. The influence of an external stellar radiation field on the coupling of the 2(3)S (upper level of the forbidden line) and 2(3)P levels (upper levels o f the intercombination lines) is taken into account. This process is mainly important for the lower-Z ions (i.e. C V, N VI, O VII) at moderate radiati on temperature (T-rad). These improved calculations were done for plasmas i n collisional ionization equilibrium, but will be later extended to photo-i onized plasmas and to transient ionization plasmas. The values for R and G are given in extensive tables, for a large range of parameters, which could be used directly to compare to the observations.