Rotating massive O stars with non-spherical 2D winds

We present solutions for the velocity field and mass-loss rates for 2D axisymmetric outflows, as well as for the case of mass accretion through the use of the Lambert W-function. For the case of a rotating radiation-driven wind the velocity field is obtained analytically using a parameterised descri...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2014-04, Vol.564, p.np-np
Hauptverfasser:	Müller, Patrick E., Vink, Jorick S.
Format:	Artikel
Sprache:	eng
Schlagworte:	Acceleration Formalism hydrodynamics Latitude Mathematical analysis Mathematical models methods: analytical methods: numerical Rotating stars: early-type stars: mass-loss stars: rotation Stellar winds Two dimensional
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!