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diskline

A line emission from a relativistic accretion disk. See Fabian et al., MNRAS 238, 729. Setting par2 to 10 is the special case of the accretion disk emissivity law ( tex2html_wrap_inline12609 ).

par1	 = 	line energy

par2 = power law depend. of emissivity (10 for disk)

par3 = inner radius (units of GM/ctex2html_wrap_inline12909 )

par4 = outer radius (units of GM/ctex2html_wrap_inline12909 )

par5 = inclination (degrees)

K = photons/cmtex2html_wrap_inline12909/s in the spectrum



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