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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 9.

[Sr/Fe] and [Y/Fe] as a function of [Fe/H] for Sculptor (left, pink) and Draco (right, blue). Pink and blue points are abundance measurements from DEIMOS, and gray arrows are upper limits. The black line is the best-fit GCE model with NSMs supplying the r-process (the same model as in Figures 3 and 4). The gray lines are GCE models with all of the same parameters, but normSrNSM and normYNSM are set to 1.

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