Non-detections at 1.3 mm from four <40 Myr exoplanets set dust mass upper limits below 10^{-4} planet mass for two disc sizes, suggesting moonetesimal formation in under 10 Myr.
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Upper limits on protolunar disc masses using ALMA observations of directly-imaged exoplanets
Non-detections at 1.3 mm from four <40 Myr exoplanets set dust mass upper limits below 10^{-4} planet mass for two disc sizes, suggesting moonetesimal formation in under 10 Myr.