On the Z-(in)dependence of the Humphreys-Davidson Limit

The temperature independent part of the Humphreys-Davidson (HD) limit sets the boundary for evolutionary channels of massive stars that either end their lives as red supergiants (RSGs) or as the hotter blue supergiants (BSGs) and Wolf-Rayet stars. Recent downward revision of most luminous RSGs the G...

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Veröffentlicht in:	Proceedings of the International Astronomical Union 2022-05, Vol.18 (S361), p.416-421
Hauptverfasser:	Sabhahit, Gautham N., Vink, Jorick S., Higgins, Erin R., Sander, Andreas A. C.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Contributed Paper Gravitational waves Helium Luminosity Magellanic clouds Massive stars Metallicity Radiation Recipes Red giant stars Stars & galaxies Stellar evolution Supergiant stars Temperature Temperature dependence Wolf-Rayet stars
Online-Zugang:	Volltext
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