Spherical galaxy collisions : Head-on encounters
We investigate low-velocity, highly interpenetrating ("hard") head-on encounters between equal mass spherical galaxies by means of full N-body simulations. We compute the energy changes (both orbital and internal) caused by the collitions strength (the perturber mass-weighted inverse of th...
Guardado en:
| Autores principales: | , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1987
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/138385 |
| Aporte de: |
| Sumario: | We investigate low-velocity, highly interpenetrating ("hard") head-on encounters between equal mass spherical galaxies by means of full N-body simulations. We compute the energy changes (both orbital and internal) caused by the collitions strength (the perturber mass-weighted inverse of the relative velocity at closes approach, Mₚ/Vₚ). Galaxies always gain energy in the encounters, but their rms velocity decreases after the collision, extra-energy being used to expand the galaxy rather than increasing its kinetic energy. The galaxies fall into bound orbits and energy rapidly if Vₚ < 2.75 σₚ, where σₚ is the rms velocity of the galaxy at maximum overlapping. |
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