Hostname: page-component-8448b6f56d-m8qmq Total loading time: 0 Render date: 2024-04-24T22:07:21.721Z Has data issue: false hasContentIssue false
  • English
  • Français

Is Stellar Wind Mass Loss During Core Hydrogen Burning Important for Evolution

Published online by Cambridge University Press:  03 August 2017

R. Blomme ,
D. Vanbeveren  and
W. Van Rensbergen
R. Blomme
Affiliation:
(1): Koninklijke Sterrenwacht, Brussels, Belgium
D. Vanbeveren
Affiliation:
(2): Dept. of Physics, VUB, Brussels, Belgium.
W. Van Rensbergen
Affiliation:
(2): Dept. of Physics, VUB, Brussels, Belgium.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The influence of wind mass loss during core hydrogen burning on the evolution of massive stars can be investigated using a relation between Ṁ-L-M-Teff based on

Type
Session VII. Evolution
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 547
Copyright
Copyright © Kluwer 1991