Dark-matter-deficient dwarf galaxies form via tidal stripping of dark matter in interactions with massive companions

In the standard ΛCDM (Lambda cold dark matter) paradigm, dwarf galaxies are expected to be dark matter-rich, as baryonic feedback is thought to quickly drive gas out of their shallow potential wells and quench star formation at early epochs. Recent observations of local dwarfs with extremely low dar...

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Bibliografski detalji
Glavni autori: Jackson, RA, Kaviraj, S, Martin, G, Devriendt, JEG, Slyz, A, Silk, J, Dubois, Y, Yi, SK, Pichon, C, Volonteri, M, Choi, H, Kimm, T, Kraljic, K, Peirani, S
Format: Journal article
Jezik:English
Izdano: Oxford University Press 2021