We obtain two-dimensional exact analytic solutions for the structure of the hot accretionflows without wind. We assume that the only non-zero component of the stress tensor is Trϕ.Furthermore, we assume that the value of ...

We implement a new semi-analytical approach to investigate radially self-similar solutions for the steady-state advection-dominated accretion flows (ADAFs). We employ the usual α-prescription for the viscosity, and all ...