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Fig. 14.


Differential chemical abundances of Si, Fe, Ni, and Ca of the analyzed stars in the tidal tails of the Hyades and NGC 2632. The color code is the same as in Fig. 7. Red crosses indicate stars identified as kinematic outliers. Shadowed regions represent the cluster signature: 1σ (dark gray) and 3σ (light gray) dispersion. Numbered stars are discussed in the text.

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