| |
Figure 1: Computational grid around the accreting center. |
| Open with DEXTER | |
![]() |
Figure 2: Contour lines of the Mach number and the temperature logarithm. Variant 1. |
| Open with DEXTER | |
![]() |
Figure 3: Contour lines of the Mach number and the temperature logarithm. Variant 2. |
| Open with DEXTER | |
![]() |
Figure 4: Contour lines of the Mach number and the temperature logarithm. Variant 3. |
| Open with DEXTER | |
![]() |
Figure 5: Contour lines of the Mach number and the temperature logarithm. Variant 4. |
| Open with DEXTER | |
![]() |
Figure 6: Contour lines of the Mach number and the temperature logarithm for the adiabatic case. Variant 15. |
| Open with DEXTER | |
![]() |
Figure 7: Streamlines and velocity vectors in the box 0<x<1,-1<z<1. Variant 2. |
| Open with DEXTER | |
![]() |
Figure 8: Streamlines in the box 0<x<20, -20<z<20. Variant 2. |
| Open with DEXTER | |
![]() |
Figure 9: Angular distributions of temperature a) and dimensionless mass flux b) through the inner boundary for Variant 2. |
| Open with DEXTER | |
![]() |
Figure 10: Dependence of the accretion rate on the efficiency of the Compton heating. The calculated rates are shown with circles, the black dot corresponds to one of the calculations of Taam et al. (1991), and the black rectangle shows the accretion rate for adiabatic accretion with parameters of Variant 2 without radiation. |
| Open with DEXTER | |
![]() |
Figure 11: Optical depth of the accreting matter as a function of the line-of-sight angle for Variant 2. |
| Open with DEXTER | |