The Einasto model is a mathematical representation used to describe the density profile of dark matter halos in galaxies. It is characterized by a smooth and continuous decline in density with increasing distance from the center of the halo, reflecting the influence of dark matter on the structure and dynamics of galaxies. This model has gained attention for providing a better fit to observational data compared to other models, such as the Navarro-Frenk-White (NFW) profile.
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