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) |
par4 | viscosity |
norm | ![]() ![]() ![]() |