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- W2114213933 abstract "Un modele de masse de galaxies spirales a deux composantes, l'une visible et l'autre sombre etendue, est developpe pour etudier la dynamique des galaxies binaires. Le potentiel gravitationnel est estime en incluant les effets du chevauchement des distributions de masse. Les orbites d'un tel systeme sont determinees. Les predictions observationnelles sont analysees avec une simulation numerique d'un echantillon de galaxies binaires." @default.
- W2114213933 created "2016-06-24" @default.
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- W2114213933 date "1990-11-01" @default.
- W2114213933 modified "2023-09-26" @default.
- W2114213933 title "BINARY GALAXIES WITH DARK HALOS .1. DYNAMICS" @default.
- W2114213933 hasPublicationYear "1990" @default.
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