Reviving old controversies: is the early Galaxy flat or round? - Investigations into the early phases of the Milky Way’s formation through stellar kinematics and chemical abundances

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Fig. 8.

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R_max − z_max plane for stars in LP sample (black dots), compared to high- and low-α stars of Nissen & Schuster sample (respectively, blue and red squares). Top panel: R_max − z_max distribution inside 20 kpc, bottom panel: distribution for the whole samples.

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