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...
Сохранить в:
| Главные авторы: | , , , |
|---|---|
| Формат: | Artigo |
| Язык: | Inglês |
| Опубликовано: |
Maynooth Academic Publishing
2025-11-01
|
| Серии: | The Open Journal of Astrophysics |
| Online-ссылка: | https://doi.org/10.33232/001c.147125 |
| Метки: |
Нет меток, Требуется 1-ая метка записи!
|