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laor

An emission line from an accretion disk around a black hole. Ari Laor's calculation including GR effects (ApJ 376, 90).

par1	 = 	Line energy in keV

par2	 = 	power law depend. of emissivity

par3	 = 	inner radius (units of   )

par4	 = 	outer radius (units of   )

par5	 = 	inclination (degrees)

K   	 = 	photons/cm/s in the line

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