Outflowing disk formation in B[e] supergiants due to rotation and bi-stability in radiation driven winds

The effects of rapid rotation and bi-stability upon the density contrast between the equatorial and polar directions of a B[e] supergiant are re-investigated. Based on a new slow solution for different high rotational radiation-driven winds and the fact that bi-stability allows a change in the line-...

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Detalles Bibliográficos
Autor principal: Rial, Diego Fernando
Publicado: 2005
Materias:
Stars: early-type
Stars: mass-loss
Stars: rotation
Stars: winds, outflows
Bifurcation (mathematics)
Ionization
Mathematical models
Optical bistability
Parameter estimation
Radiation
Temperature measurement
Velocity measurement
Stars:early-type
Stars:mass-loss
Stars:rotation
Stars:winds, outflows
Astrophysics
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v437_n3_p929_Cure
http://hdl.handle.net/20.500.12110/paper_00046361_v437_n3_p929_Cure
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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