GRB 171205A: Hypernova and Newborn Neutron Star
GRB 171205A is a low-luminosity, long-duration gamma-ray burst (GRB) associated with SN 2017iuk, a broad-line type Ic supernova (SN). It is consistent with having been formed in the core collapse of a widely separated binary, which we have called the binary-driven hypernova of type III. The core col...
Main Authors: | Yu Wang, L. M. Becerra, C. L. Fryer, J. A. Rueda, R. Ruffini |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/acb771 |
Similar Items
-
Neutron Star Binaries Produced by Binary-Driven Hypernovae, Their Mergers, and the Link between Long and Short GRBs
by: Laura M. Becerra, et al.
Published: (2023-07-01) -
GRB-SN Association within the Binary-driven Hypernova Model
by: Y. Aimuratov, et al.
Published: (2023-01-01) -
Multiwavelength Analysis of the Supernova-associated Low-luminosity GRB 171205A
by: Xiu-Juan Li, et al.
Published: (2024-01-01) -
GRB 211211A: A Neutron Star–White Dwarf Merger?
by: Shu-Qing Zhong, et al.
Published: (2023-01-01) -
Induced Gravitational Collapse, Binary-Driven Hypernovae, Long Gramma-ray Bursts and Their Connection with Short Gamma-ray Bursts
by: J. A. Rueda, et al.
Published: (2019-05-01)