Figure 4.
Sky-subtracted surface brightness profiles of the LMC clusters
Figure 4.27.
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Figure 4.26.
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Figure 4.28.
LMC 651 - 675
Sky-subtracted surface brightness profiles in logarithmic units. Once the skysubtracted profile drops below zero we terminate the plotting for that cluster. We overlay the best fit King (solid line) and EFF (long dashed line) profiles.
