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- W43360880 abstract "Presentation d'un modele hydrodynamique a 2 dimensions pour simuler l'evolution thermique et dynamique de la composante chaude du milieu interstellaire pendant une collision frontale de 2 galaxies. Le gaz contenu dans la matiere interstellaire est l'element qui souffre le plus de cette collision: si la vitesse est grande (>2.10 3 km s −1 ) c'est un gaz chaud qui quitte les galaxies; si la vitesse est moindre (10 3 km s −1 ) il se forme un disque froid qui va se lier gravitationnellement entre les 2 galaxies qui s'ecartent" @default.
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- W43360880 date "1987-01-01" @default.
- W43360880 modified "2023-09-23" @default.
- W43360880 title "Hydrodynamics of the interstellar gas in colliding galaxies. I: Head-on collisions" @default.
- W43360880 hasPublicationYear "1987" @default.
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