A modified blackbody disk model. The spectrum from the inner region of an accretion disk where the viscosity is dominated by radiation pressure.
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 | ![]() ![]() ![]() |