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 
.
|
par1 |
line energy |
|
par2 |
power law dependence of emissivity. If this parameter is 10
or greater then the accretion disk emissivity law |
|
par3 |
inner radius (units of |
|
par4 |
outer radius (units of |
|
par5 |
inclination (degrees) |
|
norm |
photon cm-2 s-1 in the spectrum |
)