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- W2062842255 abstract "High-quality observations of dark matter-dominated low surface brightness (LSB) galaxies indicate that, in contrast to the triaxial, centrally-concentrated cuspy halos formed in collisionless simulations of halo assembly, these galaxies reside in round, roughly constant density cored halos. In order to reconcile these data with galaxy formation in the context of LCDM, processes that alter the shape and density structure of the inner halo are required. We compile observational properties of LSB galaxies to evaluate the plausibility that a previously higher baryonic mass content and feedback from star formation can modify the dark matter halos of these galaxies. We also compare the properties of bulgeless disk galaxies formed in recent simulations to the LSB galaxy sample. We find that observational constraints on LSB galaxy star formation histories, structure, and kinematics make it difficult for baryonic physics to sphericalize and decrease the central density of the dark matter halos of LSB galaxies." @default.
- W2062842255 created "2016-06-24" @default.
- W2062842255 creator A5040111239 @default.
- W2062842255 creator A5050003613 @default.
- W2062842255 date "2011-10-18" @default.
- W2062842255 modified "2023-09-30" @default.
- W2062842255 title "DO BARYONS ALTER THE HALOS OF LOW SURFACE BRIGHTNESS GALAXIES?" @default.
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- W2062842255 doi "https://doi.org/10.1088/2041-8205/741/2/l29" @default.
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