Browsing by Author "Murphy, L. J."

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    Evolution of massive stars with new hydrodynamic wind models
    (2022) Gormaz-Matamala, A. C.; Cure, M.; Meynet, G.; Cuadra, J.; Groh, J. H.; Murphy, L. J.
    Context. Mass loss through radiatively line-driven winds is central to our understanding of the evolution of massive stars in both single and multiple systems. This mass loss plays a key role in modulating massive star evolution at different metallicities, especially in the case of very massive stars (M* >= 25 M-circle dot).