Dark Matter in Galaxies: Observational overview
arXiv:astro-ph/0312154
Abstract
I review the observational side of the present state of the debate about the dark matter in galaxies, with emphasis on the core/cusp problem in low surface brightness galaxies, and the question of maximum / sub-maximum disks in spiral galaxies. Some remarks are made about the dwarf spheroidals around the Milky Way, and about elliptical galaxies.
12 pages, 4 figures, includes style file, invited review at IAU Symposium 220, eds. S. Ryder, D.J. Pisano, M. Walker & K.C. Freeman, has 2 page appendix with historical notes
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Cited by in corpus (10)
- Evolution of the Bar Fraction in COSMOS: Quantifying the Assembly of the Hubble Sequence
- The universal rotation curve of dwarf disk galaxies
- Structure Formation Inside Triaxial Dark Matter Halos: Galactic Disks, Bulges and Bars
- Evidence for Dark Matter Annihilation from Galactic Gamma Rays?
- Excess of EGRET Galactic Gamma Ray Data interpreted as Dark Matter Annihilation
- Dark Matter Halos as Bose-Einstein Condensates
- Halo Geometry and Dark Matter Annihilation Signal
- Gamma ray and Neutrino fluxes from a cosmological dark matter simulation
- Quantitative interpretation of the rotation curves of spiral galaxies at redshifts z~0.7 and z~1
- The Local Universe: Galaxies in 3D