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arXiv 1997-10-09 0 views

The Quasi-stationary Structure of Radiating Shock Waves II. The Two-temperature Fluid

Sincell, M W · Gehmeyr, M · Mihalas, D

Original · EN

We solve the equations of radiation hydrodynamics in the two-temperature fluid approximation on an adaptive grid. The temperature structure depends upon the electron-ion energy exchange length, lei, and the electron conduction length, lec. Three types of radiating shock structure are observed: subcritical, where preheating of the unshocked gas is negligible; electron supercritical, where radiation preheating raises the temperature of the unshocked electron fluid to be equal to the final electron temperature; supercritical, where preheating and electron-ion energy exchange raise the preshock Tₑ,ᵢ to their final post shock values. No supercritical shock develops when lei is larger than the photospheric depth of the shocked gas because a negligible amount of the ion energy is transferred to the electrons and the shock is weakly radiating. Electron conduction smooths the Tₑ profile on a length scale lec, reducing the radiation flux.

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