Neutron Star Binaries Produced by Binary-Driven Hypernovae, Their Mergers, and the Link between Long and Short GRBs

Neutron Star Binaries Produced by Binary-Driven Hypernovae, Their Mergers, and the Link between Long and Short GRBs

The binary-driven hypernova (BdHN) model explains long gamma-ray bursts (GRBs) associated with supernovae (SNe) Ic through physical episodes that occur in a binary composed of a carbon-oxygen (CO) star and a neutron star (NS) companion in close orbit. The CO core collapse triggers the cataclysmic ev...

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Bibliographic Details
Main Authors: Laura M. Becerra, Chris Fryer, Jose F. Rodriguez, Jorge A. Rueda, Remo. Ruffini
Format: Article
Language:English
Published: MDPI AG 2023-07-01
Series:Universe
Subjects:
neutron stars
gamma-ray burst
close binaries
Online Access:https://www.mdpi.com/2218-1997/9/7/332

Internet

https://www.mdpi.com/2218-1997/9/7/332

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