next up previous contents
Next: Associated programs Up: XSPEC V10 Models Previous: zwabs

zwndabs

Photo-electric absorption from approximation to a warm absorber using Balucinska-Church and McCammon (ApJ 400, 699) cross-sections. Relative abundances are set by the abund command.

displaymath12961

where tex2html_wrap_inline12813 (E) is the photo-electric cross-section (NOT including Thomson scattering) and

par1	 = 	equivalent hydrogen column (in units of 10tex2html_wrap_inline12815 atoms/cmtex2html_wrap_inline12909 )

par2 = Window energy (keV)

par3 = redshift



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