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. Author manuscript; available in PMC: 2022 Jan 7.
Published in final edited form as: Astrophys J Lett. 2021 Jun 2;913(2):L31. doi: 10.3847/2041-8213/abfd39

Figure A1: Comparison to the model of Rafikov & Garmilla (2012).

Figure A1:

Comparing the temperature dependence of sublimative mass flux in these models for both iron and olivine (or olivine species forsterite and fayalite). These models agree to within two orders of magnitude. For iron, these two models agree closely when the T0 parameter in the Rafikov and Gamilla (2012) model is changed to match the Steckloff et al. model.