Fig. 10.
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Mass-metallicity relations for different values of total SFR, as defined in Curti et al. (2020). The SFRs of both components are the ones computed from our two-component analysis and given in Sect. 4.2.1. The markers are colour-coded with the SFR of the corresponding host galaxies. For the primary galaxy, different 3 arcsec circular apertures have been considered, as discussed in Sect. 4.7.4.
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