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            diskline: accretion disk line emission, relativistic

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 (1-sqrt(6/R))/R^3.

par1

line energy

par2

power law dependence of emissivity. If this parameter is 10 or greater then the accretion disk emissivity law (1-sqrt(6/R))/R^3 is used. Otherwise the emissivity scales as Rpar2

par3

inner radius (units of GM/c^2)

par4

outer radius (units of GM/c^2)

par5

inclination (degrees)

norm

photon cm-2 s-1 in the spectrum