Modelling The Irradiated Upper Atmospheres Of Unevolved Companions In Precataclysmic Binaries (Pcb): Evidences On Thermal Instability

Astronomy and Astrophysics – Astrophysics

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Binaries, Close-Subdwarfs, Radiative Transfer, Instability

Scientific paper

We report on our results of modelling the physical processes in the uppermost layers of strongly irradiated atmospheres of low mass unevolved companions in Precataclysmic Binaries (PCBs). Reprocessing of Lyman continuum L c radiation from the hot subdwarf (sdw) primary is studied in detail. We solve explicitly a set of equations of hydrostatic, ionization and thermal equilibrium to calculate the intensity of the reprocessed emergent radiation in recombinations for an optically thin plasma. We consider contributions from free-free and bound-free transitions. Diffuse radiation is taken into account, but the effects of self-absorption of the re-emitted radiation are neglected.

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