2003ApJ...595L..37H

We study the origin of cores and density profiles of gaseous baryonic structures in cosmology. By treating the baryons as a viscous gas, we find that both spheres and disks are possible solutions. We find analytically that the density profiles have inner and outer solutions, which in general are different. For disks, we identify a central core with a density profile ρ_d=constant and an outer profile ρ_d∼r^–3. For spherical structures, we find the profile ρ_s∼r^–6. In the presence of a dominating central black hole, we find an inner profile ρ∼r^–3/2. When the mass is dominated by a dark matter component, then the baryonic density profile will depend on the dark matter profile, and we point out how one can use this connection to infer the dark matter profile directly by observing the baryonic density profile.