laor2: accretion disk with broken-power law emissivity profile, black hole emission line

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 (Laor (1991)). 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 $GM/c^2$)
par4	outer radius (units of $GM/c^2$)
par5	inclination (degrees)
par6	radius at which emissivity power-law index changes
par7	Emissivity power-law index for radii >par6
norm	photons/cm$^2$/s in the line

HEASARC Home | Observatories | Archive | Calibration | Software | Tools | Students/Teachers/Public

Last modified: Friday, 23-Aug-2024 13:20:40 EDT