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Cited article:

Formation of supermassive stars in the first stellar clusters: Dependence on the gas temperature

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Direct Formation of Massive Black Holes via Dynamical Collapse in Metal-enriched Merging Galaxies at z ∼ 10: Fully Cosmological Simulations

Lucio Mayer, Pedro R. Capelo, Lorenz Zwick and Tiziana Di Matteo
The Astrophysical Journal 961 (1) 76 (2024)
https://doi.org/10.3847/1538-4357/ad11cf

Extreme N-emitters at high redshift: Possible signatures of supermassive stars and globular cluster or black hole formation in action

R. Marques-Chaves, D. Schaerer, A. Kuruvanthodi, D. Korber, N. Prantzos, C. Charbonnel, A. Weibel, Y. I. Izotov, M. Messa, G. Brammer, M. Dessauges-Zavadsky and P. Oesch
Astronomy & Astrophysics 681 A30 (2024)
https://doi.org/10.1051/0004-6361/202347411

Magnetic Braking during Direct Collapse Black Hole Formation

Muhammad A. Latif and Dominik R. G. Schleicher
The Astrophysical Journal Letters 952 (1) L9 (2023)
https://doi.org/10.3847/2041-8213/ace34f

Multiple Channels for Nitrogen Pollution by Metal-enriched Supermassive Stars and Implications for GN-z11

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The Astrophysical Journal Letters 949 (1) L16 (2023)
https://doi.org/10.3847/2041-8213/acd550

Direct Collapse to Precursors of Supermassive Black Hole Seeds: Radiation-feedback-generated Outflows

Yang Luo, Isaac Shlosman and Kentaro Nagamine
The Astrophysical Journal 955 (2) 99 (2023)
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Origin of supermassive black holes in massive metal-poor protoclusters

D R G Schleicher, B Reinoso, M Latif, et al.
Monthly Notices of the Royal Astronomical Society 512 (4) 6192 (2022)
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Direct collapse of exceptionally heavy black holes in the merger-driven scenario

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The low-end of the black hole mass function at cosmic dawn

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Could kilomasers pinpoint supermassive stars?

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Supermassive stars with random transverse magnetic fields

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Ionizing photon production of Population III stars: effects of rotation, convection, and initial mass function

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On monolithic supermassive stars

Lionel Haemmerlé, Alexander Heger and Tyrone E Woods
Monthly Notices of the Royal Astronomical Society 494 (2) 2236 (2020)
https://doi.org/10.1093/mnras/staa763