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Fig. 11

image

Cumulative distribution function of the distance travelled by each star normalised to the average migration. Each line indicates the migration corresponding to one of the panels in Fig. 10. Large values along the x-axis represent greater degrees of migration. Darker colours correspond to the thick disc: stars which are currently located in the range 7 <r< 8 kpc are shown in red, the ones at 10 <r< 11 kpc in blue, and the ones at 14 <r< 15 kpc in green. Lighter colours match the same radial bin but in the thin disc, with orange corresponding to our innermost bin (7 <r< 8 kpc), cyan the medium bin (10 <r< 11 kpc), and light green the outermost one (14 <r< 15 kpc).

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