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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Bibliographic Details
Main Authors: 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
Language:English
Published: Oxford University Press 2021