On Instability of a Dusty Stellar Atmosphere in Stern’s Type Configuration

Abstract

The thermal-convective instability of a stellar atmosphere in the presence of a stable solute gradient in Stern’s type configuration is studied in the presence of suspended particles. The criteria for monotonic instability are derived which are found to hold well in the presence of uniform rotation and uniform magnetic field, separately, on the thermosolutal-convective instability of a stellar atmosphere in the presence of suspended particles.