Fig. 6.
Density map of the region at positive Galactic longitude around the Sgr galaxy, for Gaia DR2 stars that have PMs within 0.5 mas yr−1 from the mean PM of the galaxy (taken from Gaia Collaboration 2018b) and colours and magnitudes compatible with being members of the Sgr dSph. The clusters associated with the main body are indicated as filled black circles and are labelled.
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