Mass fluxes for hot stars

In an attempt to understand the extraordinarily small mass-loss rates of late-type O dwarfs, mass fluxes in the relevant part of (Teff, g)-space are derived from first principles using a previously-described code for constructing moving reversing layers. From these mass fluxes, a weak-wind domain is...

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Bibliographische Detailangaben

Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2010-03, Vol.512, p.A33
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
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