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3D hydrodynamics simulations of core convection in supermassive main-sequence stars - Oxford Academic
3/22/23 at 6:12am
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Abstract. Supermassive stars are Population III stars with masses exceeding 104 M⊙ that could be the progenitors of the first supermassive black holes. Their in
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hydrodynamics simulations
core convection
Population III
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https://academic.oup.com/mnras/advance-article-abstract/doi/10.1093/mnras/stad846/7083160
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