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Fig. 7

Fig. 7 Refer to the following caption and surrounding text.

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Distribution of galactocentric total velocity (vGC) versus galactocentric radius (rGC) for stars sampled from Binney & Vasiliev (2023) model with vGC > 400km s−1 and rmin < 2.5Rh. Solid, dashed, and dotted curves show the escape-velocity profiles predicted by three Milky Way potential models: Bovy (2015), McMillan (2017), and Cautun et al. (2020).

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