Skip to main content
. Author manuscript; available in PMC: 2019 Jan 30.
Published in final edited form as: Earth Planet Sci Lett. 2017 Apr 11;467:157–166. doi: 10.1016/j.epsl.2017.02.044

Fig. 2.

Fig. 2.

Pre-exposure μ97Mo for the IAB complex iron meteorites. Shown for comparison are the μ97Mo values of primitive achondrites, magmatic iron meteorite groups, ungrouped iron meteorites, and chondrites from this study. The light grey bar is the 2SE of repeated analyses of terrestrial standards. Error bars for each sample here and in Fig. 3 are the propagated 2SD or 2SE uncertainties (see text and Table 2 for details).