Spectra and Ionization Efficiencies of Charged Decay Particles in Kilonova Ejecta
astro-ph.HE
Submitted: 2026-05-26
Updated: 2026-09-24
Terminology
Sources
- Strontium and helium in the kilonova AT2017gfo: Origin of the 1{\mu}m feature constrained via NLTE calculations
- Non-LTE Ionization Modeling for Helium and Strontium in Neutron Star Merger Ejecta
- Lanthanide Features in Near-infrared Spectra of Kilonovae
- Tellurium emission line in kilonova AT 2017gfo
- Three dimensional end-to-end simulation for kilonova emission from a black-hole neutron-star merger
- Non-LTE analysis for Helium and Strontium lines in the kilonova AT2017gfo
Related papers
- 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
- Neutrino Spectral Pinching in 3D Core-Collapse Supernovae: Late-Time Convergence, Failed-Explosion Signatures, and Viewing-Angle Dispersion