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STRUCTURAL PARAMETERS FOR 10 HALO GLOBULAR CLUSTERS IN M33

  • Authors: Jun Ma

2015 The Astronomical Journal 149 157.

  • Provider: AAS Journals

Caption: Figure 4.

Surface brightness profiles of and model fits to the sample cluster U49, with the data of the F555W and F814W bands from top to bottom. The three panels in each line from left to right are the fits to the King model (K66), Wilson model (W), and Sérsic model (S). The open squares are the data points included in the model fitting, while the crosses are points flagged as “DEP” or “BAD,” which are not used to constrain the fit. The best fitting models are shown with a red solid line. The blue dashed lines represent the shapes of the PSFs for the filters used.

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