Data for computing radiation forces on highly ionized elements

This paper gives results of an extensive computation of coefficients useful for computing radiation forces on highly ionized elements in stellar envelopes. Tables of results are provided for four different models of main-sequence stars with effective temperatures of 7240 K, 10 000 K, 12 000 K and 14 000 K. The coefficients Φ* and Ψ* defined by Alecian and Artru (1990) are obtained for 21 isoelectronic sequences (from He-like through Ti-like). A method for extrapolation toward high ionization degrees is given