Collisions of non-rotating spherical galaxies

We have used self-consistent numerical simulations of N-body systems to investigate encounters between spherical non-rotating galaxies. In our simulations, the galaxies were represented by Plummer spheres (ρ∝r–5 with isotropic velocity distribution, and we considered collisions along hyperbolic, as...

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Detalles Bibliográficos
Autores principales:	Vergne, María Marcela, Muzzio, Juan Carlos
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	1995
Materias:	Astronomía methods: numerical galaxies: evolution galaxies: interactions galaxies: structure
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/139417
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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