We explore similarities in the luminosity distribution of early type galaxies and the mass profiles of LCDM halos. The spatial structure of these systems may be accurately described by a simple law where the logarithmic slope of the projected density is a power law of radius; the Sérsic law. We show that this law provides a significantly better fit than a three-parameter generalization of the NFW profile and derive the best-fitting Sérsic parameters for a set of high-resolution LCDM halos spanning a wide range in mass. The mean Sérsic n values are 3.0 for dwarf- and galaxy-sized halos and 2.4 for cluster-sized halos, similar to the values that characterize luminous elliptical galaxies. We discuss possible reasons why the same law should describe dark and luminous systems that span a range of over seven decades in mass.
Department, Program, or Center
School of Physics and Astronomy (COS)
David Merritt et al 2005 ApJ 624 L85 https://doi.org/10.1086/430636
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This is the pre-print of an article published by the American Astronomical Society. The final, published version is available here: https://doi.org/10.1086/430636
© 2005 The American Astronomical Society
Also archived in: arXiv: astro-ph/0502515 v1 24 Feb 2005
DM was supported by grants AST-0206031, AST-0420920 and AST-0437519 from the NSF and grantNNG04GJ48G fromNASA. JFN acknowledges support fromthe Alexander von Humboldt Foundation.
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