An approximate NLTE opacity scheme using Sobolev escape probabilities and a 4-million-line database enables RHD simulations of hot star winds that develop multi-component temperature structures from shock heating and radiative cooling.
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Multi-dimensional, time-dependent approximate NLTE unified model atmospheres with winds for hot, massive stars
An approximate NLTE opacity scheme using Sobolev escape probabilities and a 4-million-line database enables RHD simulations of hot star winds that develop multi-component temperature structures from shock heating and radiative cooling.