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. Author manuscript; available in PMC: 2019 Apr 30.
Published in final edited form as: Astrophys J Lett. 2018 Mar 18;856(2):L24. doi: 10.3847/2041-8213/aab61f

Figure 2.

Figure 2.

Measured 54Cr/52Cr ratios as a function of grain diameter for fourteen 54Cr-rich grains for which SEM analysis indicated that they were fully spatially resolved. Black curve indicates approximate 4σ detection limit, the criterion used here to identify a grain as isotopically anomalous. Error bars are 1σ.