Self-consistent modelling of line-driven hot-star winds with Monte Carlo 
radiation hydrodynamics

Noebauer, U. M.; Sim, S. A.

doi:10.1093/mnras/stv1849

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Self-consistent modelling of line-driven hot-star winds with Monte Carlo radiation hydrodynamics

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Noebauer, U. M.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Noebauer, U. M., & Sim, S. A. (2015). Self-consistent modelling of line-driven hot-star winds with Monte Carlo radiation hydrodynamics. Monthly Notices of the Royal Astronomical Society, 453(3), 3120-3134. doi:10.1093/mnras/stv1849.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0029-2193-9

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