Occurrence of Gravitational Collapse in the Accreting Neutron Stars of Binary-driven Hypernovae

Occurrence of Gravitational Collapse in the Accreting Neutron Stars of Binary-driven Hypernovae

The binary-driven hypernova (BdHN) model proposes long gamma-ray bursts (GRBs) originate in binaries composed of a carbon–oxygen (CO) star and a neutron star (NS) companion. The CO core collapse generates a newborn NS and a supernova that triggers the GRB by accreting onto the NSs, rapidly transferr...

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Bibliographic Details
Main Authors: L. M. Becerra, F. Cipolletta, C. L. Fryer, Débora P. Menezes, Constança Providência, J. A. Rueda, R. Ruffini
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Gamma-ray bursts
Neutron stars
Black holes
Gravitational collapse
Core-collapse supernovae
Close binary stars
Online Access:https://doi.org/10.3847/1538-4357/ad82ea

Internet

https://doi.org/10.3847/1538-4357/ad82ea

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