Fig. 2

PDF of the birth Galactocentric radius (left) and of the age (right) of HD 19467 derived using an evolution model of the MilkyWay (see text). In both panels, the red thick curves show the best-fit and the gray curves are drawn using the uncertainties in the model parameters. In the right panel, the red dashed curve represents the age PDF assuming only that HD 19467 belongs to the Milky Way disk.
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