GRB-SN Association within the Binary-driven Hypernova Model

GRB-SN Association within the Binary-driven Hypernova Model

Observations of supernovae (SNe) Ic occurring after the prompt emission of long gamma-ray bursts (GRBs) are addressed within the binary-driven hypernova (BdHN) model where GRBs originate from a binary composed of a ∼10 M _⊙ carbon–oxygen (CO) star and a neutron star (NS). The CO core collapse gives...

Full description

Bibliographic Details
Main Authors: Y. Aimuratov, L. M. Becerra, C. L. Bianco, C. Cherubini, M. Della Valle, S. Filippi, Liang Li, R. Moradi, F. Rastegarnia, J. A. Rueda, R. Ruffini, N. Sahakyan, Y. Wang, S. R. Zhang
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Gamma-ray bursts
Online Access:https://doi.org/10.3847/1538-4357/ace721

Internet

https://doi.org/10.3847/1538-4357/ace721

Similar Items