Fig. 7
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Streams of stars in the D–Λ⊙ space at present color-coded by the ejection time. The solid black curve represents the distance trend of the Vasiliev et al. (2021) stars, while the shaded region is the distance error, both quantities being moving means as a function of the longitude, Λ⊙. The distances are referred to the Galactocentric reference frame.
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