An extensive grid of mass fluxes for Galactic O stars

A previously-described code for constructing moving reversing layers (MRL) is improved by replacing a two-parameter model for gl(v), the radiative acceleration due to lines, with a flexible non-parametric description, thus allowing a greater degree of dynamical consistency in modelling turbulent tra...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2010-12, Vol.524, p.A41
1. Verfasser:	Lucy, L. B.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Earth, ocean, space Exact sciences and technology outflows stars: early-type stars: mass-loss stars: winds
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!