The peculiar abundances of HE 1005–1439 - A carbon-enhanced extremely metal-poor star contaminated with products of both s- and i-process nucleosynthesis

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Fig. 5.

Examples of theoretical model fits with the observed abundances of the star. In panels a, b, and c, the points with error bars indicate the observed abundances. (a) s-process model fits for M = 1.3 M_⊙ & 2.0 M_⊙. (b) i-process model fits for n = 10¹² cm⁻³ and 10¹⁴ cm⁻³. (c) Best-fit from parametric-model. (d) Residual plot.

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