The age, kinematics, and metallicity of nearby Sun-like stars and the history of the Milky Way disc

Open Access

Fig. 3.

Age distributions derived by inverting the index distributions of all sample stars. The grey areas represent the ±1σ envelopes of 1000 realisations of the age distributions assuming Gaussian distributions of the mass and average index of each star around the average values provided in the AMBRE-HARPS catalogue of indices with the uncertainties given in the catalogue.

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