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- W2081454639 abstract "Etude du vent stellaire de la primaire du systeme binaire V861 Sco a partir de donnees du satellite IUE. Les profils P Cygni observes montrent une correlation entre la vitesse maximum et le potentiel d'ionisation. Les resultats correles a un modele de bilan d'ionisation dans le vent permettent de deriver un taux de perte de masse de 3•10 −6 M ○. an −1" @default.
- W2081454639 created "2016-06-24" @default.
- W2081454639 creator A5078510529 @default.
- W2081454639 date "1984-11-01" @default.
- W2081454639 modified "2023-09-24" @default.
- W2081454639 title "An analysis of V861 Sco – II. The stellar wind" @default.
- W2081454639 doi "https://doi.org/10.1093/mnras/211.1.167" @default.
- W2081454639 hasPublicationYear "1984" @default.
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