An Explanation for the Slopes of Stellar Cusps in Galaxy Spheroids [PDF]
Philip F. Hopkins, Eliot QuataertThe stellar surface mass density profiles at the centers of typical ~L* and lower-mass spheroids exhibit power law 'cusps' with $\Sigma \propto R^(-n)$, where 0.5View original: http://arxiv.org/abs/1011.3045
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