arXiv (All)
open access
Waiting in the wings: extended emission GRBs from high latitude emission and jet expansion
The process powering extended emission (EE) Gamma Ray-Bursts (GRBs) from compact object mergers is a debated problem due to their observed prompt emission timescales of 10 to 100s, far in excess of the expected accretion timescales following a binary neutron star (BNS) merger. Here, we present an an
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Multi-scale variability in the optical afterglow of GRB 251013C from high-cadence LAST observations#1051835
- Timing-Window Mechanism for Chain-Like Transients in Collisions of Radially Excited Boson Stars#987677
- Determination of the Angular Distributions of Dynamical and Emission Parameters of GRB Relativistic Outflows#1110699
- Spheroidal Resampling Analysis of High-Redshift Gamma-Ray Burst Spatial Densities#999862
- The wave normals of ELF hiss emissions observed onboard GEOS 1 at the equatorial and off‐equatorial regions of the plasmasphere#377899
Record · ID 1063121
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive