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Fig. 22
Surface brightness profile compiled from archival HST ACS data (black stars) of the EO VUCD7 and the surface brightness profile of model CC_56_60-kpc (grey line) from Brüns et al. (2011) using a mass-to-light ratio of 2.8. The model and the observed EO show a very similar two-component or “core-halo” structure.
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