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. Author manuscript; available in PMC: 2021 Nov 12.
Published in final edited form as: Geochim Cosmochim Acta. 2021 Feb 18;299:199–218. doi: 10.1016/j.gca.2021.02.012

Fig. 8.

Fig. 8.

Δ17O values vs. Mg#s of individual host chondrules in CM (open diamonds; Chaumard et al., 2018; this work), CO (grey circles; Tenner et al., 2013), and Acfer 094 (black circles; Ushikubo et al., 2012) chondrites. Chondrule Mg# uncertainties correspond to the range of measured values, while uncertainties in Δ17O are the propagated 2SE.