Analytical solutions for radiation-driven winds in massive stars II : The δ-slow regime

Accurate mass-loss rates and terminal velocities from massive stars winds are essential to obtain synthetic spectra from radiative transfer calculations and to determine the evolutionary path of massive stars. From a theoretical point of view, analytical expressions for the wind parameters and veloc...

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Detalles Bibliográficos
Autores principales:	Araya, I., Christen, A., Curé, Michel, Cidale, Lydia Sonia, Venero, Roberto Oscar José, Arcos, C., Gormaz Matamala, A. C., Haucke, Maximiliano, Escarate, P., Clavería, H.
Formato:	Articulo Preprint
Lenguaje:	Inglés
Publicado:	2021
Materias:	Ciencias Astronómicas Física hydrodynamics methods: analytical stars: early-type stars: mass-loss stars: winds, outflows
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/124521
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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