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astro-ph.SR2026
Turbulent viscosity in line-driven stellar winds
Matías Montesinos, Michel Cure, Ignacio Araya +1
Radiation-driven winds from massive stars generate powerful outflows known to be intrinsically turbulent. Despite this, standard hydrodynamic models have historically restricted th…
astro-ph.SR2026
Line-driven Radiative Winds in B-Supergiants: Bridging the Gap between Fast and Slow m-CAK Solutions
Matías Montesinos, Emil Zabala-Arroyo, Juan José Castro-Salgado +2
The modified Castor, Abbott, and Klein (m-CAK) theory predicts different wind regimes based on the line force parameter for changes in ionization () and the rotation parameter (…