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            disko: accretion disk, inner, radiation pressure viscosity

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

2cos(i)/d^2 where i is the inclination of the disk and d is the distance in units of 10 kpc