“School of Astronomy”
Back to Papers HomeBack to Papers of School of Astronomy
| Paper IPM / Astronomy / 14803 |
|
||||||
| Abstract: | |||||||
|
We obtain two-dimensional exact analytic solutions for the structure of the hot accretion flows without wind. We assume that the only non-zero component of the stress tensor is Tr�?. Furthermore we assume that the value of viscosity coefficient ñ varies with ø. We find radially self-similar solutions an compare them with the numerical and the analytical solutions already studied in the literature. The no-wind solution obtained in this paper may be applied to the nuclei of some cool-core clusters
Download TeX format |
|||||||
| back to top | |||||||
