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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 2.

Abundance profiles of the 7000 M⊙ star at three evolutionary stages. Top: beginning of core He burning. Middle: middle of core He burning. Bottom: end of Si burning. Purple and yellow regions mark convective and radiative zones, respectively.

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