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Cited article:

Rotating supermassive Pop III stars on the main sequence

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

Devesh Nandal, Daniel J. Whalen, Muhammad A. Latif and Alexander Heger
The Astrophysical Journal Letters 994 (1) L11 (2025)
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The evolution of accreting population III stars at 10−6–103 M⊙ yr−1

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Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels

Boyuan Liu, Tilman Hartwig, Nina S Sartorio, Irina Dvorkin, Guglielmo Costa, Filippo Santoliquido, Anastasia Fialkov, Ralf S Klessen and Volker Bromm
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The earliest phases of CNO enrichment in galaxies

M. Rossi, D. Romano, A. Mucciarelli, E. Ceccarelli, D. Massari and G. Zamorani
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Explaining the high nitrogen abundances observed in high-z galaxies via population III stars of a few thousand solar masses

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Astronomy & Astrophysics 683 A156 (2024)
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Towards a universal analytical model for Population III star formation: interplay between feedback and fragmentation

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Rapidly rotating Population III stellar models as a source of primary nitrogen

Sophie Tsiatsiou, Yves Sibony, Devesh Nandal, Luca Sciarini, Yutaka Hirai, Sylvia Ekström, Eoin Farrell, Laura Murphy, Arthur Choplin, Raphael Hirschi, Cristina Chiappini, Boyuan Liu, Volker Bromm, Jose Groh and Georges Meynet
Astronomy & Astrophysics 687 A307 (2024)
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