Phenomenological distribution of dark matter halos of galaxy comprising of stellar streams
Using the potential associated with NFW mass profile (Navarro et al. in Mon. Not. R. Astron. Soc. 402:21, 2010) enclosed at scale radius rₛ, we calculate the partition function of the clustering of dark halos comprising of stellar streams, which are the outcome of accretion of globular clusters or d...
Guardado en:
| Autores principales: | Hameeda, Mir, Rocca, Mario Carlos |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2021
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/136429 |
| Aporte de: |
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