Including a constant turbulent pressure in 1D O-star atmosphere models reproduces 2D-simulated density stratifications and lowers the spectroscopic mass discrepancy.
C., Lanz , T., Hillier , D
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Improving 1D stellar atmosphere models with insights from multi-dimensional simulations I. 1D vs 2D stratifications and spectral comparison for O stars
Including a constant turbulent pressure in 1D O-star atmosphere models reproduces 2D-simulated density stratifications and lowers the spectroscopic mass discrepancy.