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Constraints on the r-process Delay Time from Dwarf Spheroidal Galaxies

  • Authors: Lauren E. Henderson, Evan N. Kirby, Mithi A. C. de los Reyes, Rebecca Surman

Lauren E. Henderson et al 2026 The Astrophysical Journal 1011 .

  • Provider: AAS Journals

Caption: Figure 5.

[Sr/Fe], [Y/Fe], [Ba/Fe], [Eu/Fe], and [Ba/Eu] as a function of [Fe/H] in Sculptor. Pink points are abundance measurements. Gray arrows are upper limits. [Ba/Eu] error bars are from [Ba/Fe] and [Eu/Fe] errors added in quadrature, with only combined errors < 0.5 shown. The light gray, gray, and black lines are the best-fit GCE models for the r-process tests given in Table 3.

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