On the source of dense outflows from T Tauri stars -I. Photoionization of cool MHD disc winds
Cool magnetohydrodynamics (MHD) disc wind physics is reviewed by means of a self-similar analytical model, putting special emphasis on the mathematical aspects of the solution. It is found that the key parameter of the theory (μ.) measures the relation between magnetic and tidal forces. The generati...
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2003
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v342_n2_p427_FerroFontan http://hdl.handle.net/20.500.12110/paper_00358711_v342_n2_p427_FerroFontan |
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