Paper detail

Exact analytical solutions for ADAFs

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 $T_{rφ}$. Furthermore we assume that the value of viscosity coefficient $α$ varies with $θ$. We find radially self-similar solutions and 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.