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- W53454964 abstract "L'effondrement axisymetrique des proto-galaxies en rotation est etudie numeriquement par application de l'equation hydrodynamique d'Euler pour la composante gazeuse et d'un modele anisotrope pour le systeme stellaire. Les resultats des simulations montrent la formation d'un halo spheroidal pauvre en metal et d'un disque galactique riche en metal, mais ne montrent pas la formation d'un bulbe galactique. Les modeles montrent une forte correlation entre la taille du disque galactique et le parametre de spin initial λ, suggerant que les galaxies elliptiques pourraient se former a partir de proto-galaxies avec λ petit et les galaxies spirales avec λ initial plus eleve" @default.
- W53454964 created "2016-06-24" @default.
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- W53454964 date "1988-06-01" @default.
- W53454964 modified "2023-09-26" @default.
- W53454964 title "Anisotropic models of galactic evolution" @default.
- W53454964 hasPublicationYear "1988" @default.
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