An emission line from an accreti on disk with a broken power-law emissivity profile around a black hole. Uses Ari Laor's calculation including GR effects (ApJ 376, 90). Modified from laor model by Andy Fabian.
|
par1 |
Line energy in keV |
|
par2 |
Index: power law dependence of emissivity (scales as R–Index) |
|
par3 |
inner radius (units of |
|
par4 |
outer radius (units of |
|
par5 |
inclination (degrees) |
|
par6 |
radius at which emissivity power-law index changes |
|
par7 |
Emissivity power-law index for radii > par6 |
|
norm |
photons cm–2s-1 in the line |
