Magnetohydrodynamic stellar winds: A new class of solutions
This paper introduces a new class of analytic MHD solutions for steady, axisymmetric, rotating outflows interacting with poleward deflected, partially open magnetic fields. In the first paper of this series, several simplifying assumptions were necessary to deal with the problem in an analytical fas...
Guardado en:
| Publicado: |
1995
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v449_n2_p764_Rotstein http://hdl.handle.net/20.500.12110/paper_0004637X_v449_n2_p764_Rotstein |
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