Erratum: “Tidal Spin-up of Black Hole Progenitor Stars” (2023, ApJ, 952, 53)
Authors: Linhao Ma, 昊 马林, Jim Fuller
Linhao Ma et al
2024 The Astrophysical Journal965.
Provider: AAS Journals
Caption: Figure 9.
The dimensionless spin of resulting BHs for our W-R star models with the nonlinear damping rates we estimate in Appendix D in the published article. Zahn’s predictions are also shown. The BH spins are significantly increased when including nonlinear damping, especially for high-mass BHs and short-period systems. Hence, nonlinear effects could be an important factor in these systems.