A photoelectric absorption with variable abundances using Balucinska-Church and McCammon (ApJ 400, 699) cross-sections. The relative abundances are set by the abund command. This model is identical to varabs except for the way that the parameters are defined.
where is the photo-electric cross-section (NOT including
Thomson scattering) and
par1 = equivalent hydrogen column (in units ofatoms/cm
)
par2-par18 = abundances for He, C, N, O, Ne, Na, Mg, Al, Si, S,
Cl, Ar, Ca, Cr, Fe, Co, Ni wrt to Solar (defined by the abund command)