Synthesis of thorium and uranium in asymptotic giant branch stars

Open Access

Fig. 3.

Best fits to the abundances of the CEMP r/s star RAVE J094921.8−161722 (Gull et al. 2018) using the five AGB models listed in Table 1. The abundance of uranium is based on the ²³⁸U isotope only; the ²³⁵U isotope, with a half-life of t_1/2 = 0.7 Gyr, was assumed to have fully decayed.

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