Two-phase radiative/conductive equilibrium in AGN and GBH

We determine simple analytical conditions for combined radiative and thermal equilibrium between the X-ray emitting plasma and cold reprocessor in active galactic nuclei (AGN) and galactic black holes (GBH). These conditions determine the pressure at the transition zone, which is not arbitrary in the static situation. The conditions for static solution are derived analytically for different forms of plasma heating and for cooling provided by Compton cooling, bremsstrahlung, and (optionally) advective cooling. We conclude that if Compton heating is the only heating mechanism, we always achieve static equilibrium between the phases. For constant volume heating and radiatively cooled plasma the static solution is never achieved and evaporation or condensation takes place. However, static solutions with no evaporation/condensation are found for radiative cooling supplemented with lateral advection. Similar results are obtained for a two-temperature plasma. In the case of a general prescription of mechanical heating (Q = hoP mT−s) of radiatively-cooled one-temperature plasma, we found that static solution is only possible, when 0 < s < 3/2. Such conditions apply to all models, like disc/corona solutions, ADAF flows at their outer ADAF/disc boundary or cold clumps embedded in a hot medium. These models have to be reconsidered and supplemented either with additional condition for the pressure at the transition zone or with equation describing the mass exchange between the phases.