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Fig. 6.


LOSVD of the bright component (grey histogram with errorbars) in the north (top) and south (bottom) of the galaxy. The northern component is best-fit by a single Gaussian (solid black line). The substructure of VCC 1249 in the southern part is fit by a Gaussian (dotted red line) in addition to the halo (dashed blue line). While the likelihood is fit with a bin-free method, we bin the LOSVDs for visual convenience.

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