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zvphabs

A redshifted photoelectric absorption with variable abundances using Balucinska-Church and McCammon (ApJ 400, 699) cross-sections. The abundances are specified relative to the Solar abundance table set using the abund command. This model is identical to zvarabs except for the way that the parameters are defined.

displaymath12945

where tex2html_wrap_inline12531 is the photo-electric cross-section (NOT including Thomson scattering) and

par1	   =  	equivalent hydrogen column (in units of  tex2html_wrap_inline12819 atoms/cmtex2html_wrap_inline12909 )

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)

par19 = redshift



Keith Arnaud (kaa@genji.gsfc.nasa.gov)
Wed May 28 10:59:33 EDT 1997