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Fig. 5

image

[Fe/H] of RGB stars as a function of angular distance from Sgr core along the leading stream (left panels) and trailing stream (right panels). The upper panels show the individual RGB stars. In the lower panels, the distribution of [Fe/H] is displayed as the median. The solid line shows the result of a least-squares linear fit to the median data of RGB stars.

This figure is made of several images, please see below:

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