Efectos de mareas en cúmulos globulares
Abstract. Using an N-body numerical simulation in the framework of the ΛCDM cosmological model we study the globular cluster population in a simulated galaxy cluster. We select particles that trace the bimodal (red and blue) globular cluster system of each individual dark matter halo prior to their...
Guardado en:
| Autores principales: | , , , |
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| Formato: | publishedVersion conferenceObject |
| Lenguaje: | Español |
| Publicado: |
Asociación Argentina de Astronomía
2021
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| Materias: | |
| Acceso en línea: | http://hdl.handle.net/11086/18996 |
| Aporte de: |
| Sumario: | Abstract. Using an N-body numerical simulation in the framework of the ΛCDM cosmological model we study the globular cluster population in a simulated galaxy cluster. We select particles that trace the bimodal (red and blue) globular cluster system of each individual dark matter halo
prior to their incorporation to the cluster virial radius. We found that the blue population is more prone to be removed from the halo than the red one. This result suggests that globular clusters are tidally disrupted,
being the blue (more extended) population easily removed. |
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