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- W210465967 abstract "Une grille de modeles de vents stellaires le long des traces d'evolution des etoiles O massives est calculee en utilisant une theorie amelioree du vent entretenu par le rayonnement. Les resultats montrent que ces modeles peuvent decrire le comportement observe des profils de la raie Si IV par rapport a ceux de C IV et N V comme fonction du type spectral et de la classe de luminosite. De plus, une sequence de profils de la raie O VI est calculee, indiquant que la theorie est capable de produire les structures P-Cygni jusqu'aux temperatures effectives d'environ 41000 K" @default.
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- W210465967 date "1990-02-01" @default.
- W210465967 modified "2023-09-23" @default.
- W210465967 title "Radiation driven winds of hot luminous stars. VII: The evolution of massive stars and the morphology of stellar wind spectra" @default.
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