Figure 7.
95% (light bars) and 68% (dark bars) posterior intervals from our final abundance study. Total elemental abundances are in orange, while individual isotopes are in green. We show the latest determination of the solar photospheric (blue dots) elemental abundances and errors from Asplund et al. (2009), with updated heavier (A ⩾ 23) elemental abundances from Scott et al. (2015). We also show previously used values from GALPROP (Moskalenko et al. 2008) with open black circles.
