most citedLow-mass Pop III star formation due to the HD-cooling induced by weak Lyman-Werner radiation

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astro-ph.GA2023★ 1 cited

Low-mass Pop III star formation due to the HD-cooling induced by weak Lyman-Werner radiation

Sho Nishijima, Shingo Hirano, Hideyuki Umeda

Lyman-Werner (LW) radiation photodissociating molecular hydrogen (H) influences the thermal and dynamical evolution of the Population III (Pop III) star-forming gas cloud. The…