A new numerical method for solving radiation driven winds from hot stars

We present a general method for solving the non-linear differential equation of monotonically increasing steady-state radiation driven winds. We graphically identify all the singular points before transforming the momentum equation to a system of differential equations with all the gradients explici...

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Detalles Bibliográficos
Autores principales: Curé, M., Rial, D.F.
Formato: JOUR
Materias:
Hydrodynamics
Methods: analytical
Stars: early-type
Stars: mass-loss
Stars: winds, outflows
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046337_v328_n6_p513_Cure
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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