A Shell Collision Scenario for EP251222b/GRB 251222A: Connecting Prompt Emission and Double-Peaked Afterglow
astro-ph.HE
Submitted: 2026-10-15
Updated: 2026-10-15
Comments: 26 pages, 9 figures. Submitted to The Astrophysical Journal (ApJ)
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Related papers
- Accreting Neutron Stars in Low-Mass X-ray Binaries
- Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
- Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole
- Impact of Magnetic Field Topology on Electromagnetic and Gravitational Waves from Binary Neutron Star Merger Remnants
- XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary
- SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics