Magnetohydrodynamic stellar wind solutions in curved magnetic fields

This paper generalizes the analytic class of magnetohydrodynamic (MHD) solutions introduced by Low and Tsinganos for steady, rotating, axisymmetric stellar winds embedded in partially open magnetic fields. The collimation of the outflow is achieved by assuming a magnetic configuration that not only...

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Detalles Bibliográficos
Autores principales: Rotstein, N.O., Fontán, C.F.
Formato: JOUR
Materias:
MHD
Plasmas
Stars: mass loss
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0004637X_v449_n2_p745_Rotstein
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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