A disk model with gas pressure viscosity. The spectrum from an accretion disk where the viscosity scales as the gas pressure. From Stella and Rosner (1984).
|par1||accretion rate in Eddington Luminosities|
|par2||central mass in solar mass units|
|par3||inner disk radius in gravitational (= 3 Schwarzschild radii)|
|norm||where is the inclination of the disk and is the distance in units of 10 kpc|