Fig. 7
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Carbon-to-oxygen ratio of GQ Lup B compared to other young substellar companions (<100 Myr). The solar value and its uncertainty are shown as a grey band. The size of the markers is proportional to the mass. The data used to create this figure and their uncertainties can be found in Petrus et al. (2021), Zhang et al. (2021a), Lacour et al. (2021), Dupuy et al. (2023), Gandhi et al. (2023), Hoch et al. (2023), Brown-Sevilla et al. (2023), Mesa et al. (2023), Palma-Bifani et al. (2023), Palma-Bifani et al. (2024), Landman et al. (2024) and Costes et al. (2024).
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