Аккреционные диски. ... C- code to calculate evolution of the accretion disk with time-independent viscosity in a binary system (v0.3 March 2015) ( см. ... Observed flux F=L*Psi(theta)/(4 pi D)^2, where L is the bolometric luminosity, D is the distance to the disk, theta is the angle between the normal to the disk plane and the line of sight, mu = cos(theta), mu=0 when photons go parallel to the disk plane. a=0.0 ; a=0.9981 ; Functions are calculated using different codes: kerrbb ( Li et al., ...