Dynamical friction and measurements of the splashback radius in galaxy clusters
The splashback radius is one popular method of constraining the size of galaxy clusters, often measured through the logarithmic derivative of the galaxy number density profile. However, measuring the splashback radius through the galaxy number density has consistently produced smaller values of the...
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| Principais autores: | , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Maynooth Academic Publishing
2025-11-01
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| coleção: | The Open Journal of Astrophysics |
| Acesso em linha: | https://doi.org/10.33232/001c.147125 |
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