On the dark matter content of ultra-diffuse galaxies
I compare the dark matter content within stellar half-mass radius expected in a $\Lambda$CDM-based galaxy formation model with existing observational estimates for the observed dwarf satellites of the Milky Way and ultra-diffuse galaxies (UDGs). The model reproduces the main properties and scaling r...
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| Format: | Article |
| Language: | English |
| Published: |
Maynooth Academic Publishing
2024-12-01
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| Series: | The Open Journal of Astrophysics |
| Online Access: | https://doi.org/10.33232/001c.127487 |
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