The Evolutionary history of the Milky Way discs and halo from Gaia DR2 colour-magnitude diagram fitting
The technique of color-magnitude diagram (CMD) fitting is a well recognized method that has been used for over 20 years to determine detailed star formation histories (SFH) for Local Group galaxies (Gallart et al. 2005; Tolstoy et al. 2009). The accurate distances for large stellar samples provided in Gaia DR2, together with the precise
Gallart, Carme et al.
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2019