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1000–10,000 M⊙ Primordial Stars Created the Nitrogen Excess in GS 3073 at z = 5.55

  • Authors: Devesh Nandal, Daniel J. Whalen, Muhammad A. Latif, Alexander Heger

Devesh Nandal et al 2025 The Astrophysical Journal Letters 994 .

  • Provider: AAS Journals

Caption: Figure 6.

Left: evolution of central densities versus central temperatures. The gray shaded zone is the PI regime. A few models such as the 6000, 7000, and 8000 M⊙ stars were evolved past the PI into core Si burning. Right: collapse of the 8000 M⊙ star to a BH.

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