The Relevance of Dynamical Friction for the MW/LMC/SMC Triple System
Simulations of structure formation in the standard cold dark matter cosmological model quantify the dark matter halos of galaxies. Taking into account dynamical friction between dark matter halos, we investigate the past orbital dynamical evolution of the Magellanic Clouds in the presence of the Gal...
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| Hauptverfasser: | , |
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| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
MDPI AG
2024-03-01
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| Schriftenreihe: | Universe |
| Schlagworte: | |
| Online-Zugang: | https://www.mdpi.com/2218-1997/10/3/143 |
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