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Where Has All the R-process Gone? Timescales for Gamma-Ray Burst Kilonovae to Enrich Their Host Galaxies

  • Authors: Anya E. Nugent, Alexander P. Ji, Wen-fai Fong, Hilay Shah, Freeke van de Voort

Anya E. Nugent et al 2025 The Astrophysical Journal 982 .

  • Provider: AAS Journals

Caption: Figure 5.

An illustration of penrich and how it is affected by the host’s SFH. In the “high” penrich example, a substantial fraction of stellar mass is produced after zenrich in the host compared to the amount of stellar mass formed before zenrich. In the “low” penrich example, the amount of stellar mass produced after zenrich is small in comparison to the amount formed before.

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