The evolution of rotating very massive stars with LMC composition

Context. With growing evidence for the existence of very massive stars at subsolar metallicity, there is an increased need for corresponding stellar evolution models. Aims. We present a dense model grid with a tailored input chemical composition appropriate for the Large Magellanic Cloud (LMC). Meth...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2015-01, Vol.573, p.A71
Hauptverfasser:	Köhler, K., Langer, N., de Koter, A., de Mink, S. E., Crowther, P. A., Evans, C. J., Gräfener, G., Sana, H., Sanyal, D., Schneider, F. R. N., Vink, J. S.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Combustion Magellanic clouds Massive stars Metallicity Stars stars: abundances stars: early-type stars: evolution stars: massive stars: rotation Stellar evolution Supernovae
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!