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. 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. 4.

Fig. 4.

Idealized IAB complex parent bodies with the preferred formation mechanisms for the MG and each of the subgroups, combining evidence from Mo and W isotope data (this study) with HSE data and observed silicate distributions among MG irons (Worsham et al., 2016a). Winonaites likely formed on the MG-sLL parent body (McCoy et al., 1993; Benedix et al., 2000). Relative parent body sizes are arbitrary.