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. Author manuscript; available in PMC: 2017 Jun 2.
Published in final edited form as: Astrophys J Suppl Ser. 2017 Jan 20;228(1):10. doi: 10.3847/1538-4365/228/1/10

Figure 3.

Figure 3

Solar photospheric abundances for Cr I and Cr II lines plotted as functions of wavelength (panel (a)) and excitation potential (panel (b)). The statistics for the mean abundances for Cr I (red dots) and Cr II (blue x’s) are written in panel (a). In each panel blue solid lines indicate the mean Cr II abundance, and blue dotted lines indicate ±σ deviations from the mean.