Gamma-Ray Bursts: To be Short or Long is not the Question
arXiv:2111.13379 · doi:10.1038/s41550-021-01401-4
Abstract
The association of a short gamma-ray burst with a core-collapse supernova seems to challenge current scenarios for the origin of these extreme events. But how much can we rely on observed duration for pinpointing their progenitors?
arXiv comment2 pages, 1 figure, published in Nature Astronomy - News and Views section; published version available at the journal website link https://rdcu.be/cpVCE
References in corpus (11)
- Multi-messenger Observations of a Binary Neutron Star Merger
- Discovery of the peculiar supernova 1998bw in the error box of GRB980425
- The Supernova -- Gamma-Ray Burst Connection
- Short-Duration Gamma-Ray Bursts
- Discovery of the X-Ray Afterglow of the Gamma-Ray Burst of February 28 1997
- Theories of Gamma-Ray Bursts
- Swift detects a remarkable gamma-ray burst, GRB 060614, that introduces a new classification scheme
- Short vs Long and Collapsars vs. non-Collapsar: a quantitative classification of GRBs
- Discovery and confirmation of the shortest gamma ray burst from a collapsar
- A Peculiarly Short-duration Gamma-Ray Burst from Massive Star Core Collapse
- Long-Duration Gamma-Ray Burst Host Galaxies in Emission and Absorption
Cited by in corpus (6)
- The peculiar short-duration GRB 200826A and its supernova
- GRB minimum variability timescale with Insight-HXMT and Swift: implications for progenitor models, dissipation physics and GRB classifications
- Two Dimensional Clustering of Gamma-Ray Bursts using durations and hardness
- GRB 201015A and the nature of low-luminosity soft gamma-ray bursts
- In search of short gamma-ray burst optical counterpart with the Zwicky Transient Facility
- Characterization of the GRB prompt fundamental plane using Fermi-GBM data