Low-mass Population III Star Formation due to the HD Cooling Induced by Weak Lyman–Werner Radiation

Low-mass Population III Star Formation due to the HD Cooling Induced by Weak Lyman–Werner Radiation

Lyman–Werner (LW) radiation photodissociating molecular hydrogen (H _2 ) influences the thermal and dynamical evolution of the Population III (Pop III) star-forming gas cloud. The effect of powerful LW radiation has been well investigated in the context of supermassive black hole formation in the ea...

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Bibliographic Details
Main Authors: Sho Nishijima, Shingo Hirano, Hideyuki Umeda
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Hydrodynamical simulations
Population III stars
Star formation
Online Access:https://doi.org/10.3847/1538-4357/ad2fc9

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