New Constraints on r-process Nucleosynthesis in Neutron Star Mergers from GW170817 Late-Phase Spectra
astro-ph.HE
Submitted: 2026-09-30
Updated: 2026-09-30
Terminology
Sources
- Strontium and helium in the kilonova AT2017gfo: Origin of the 1{\mu}m feature constrained via NLTE calculations
- Atomic Data for Non-Equilibrium Modeling of Kilonovae: The Ionization Properties of Te I - III
- Non-LTE Ionization Modeling for Helium and Strontium in Neutron Star Merger Ejecta
- Heavy element dust explains the late-time spectra of kilonovae
- Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars
- Calibrated Lanthanide Atomic Data for Kilonova Radiative Transfer. I. Atomic Structure and Opacities
- Improved lanthanide constraints for the kilonova AT 2017gfo
- Heavy element nucleosynthesis associated with a gamma-ray burst
- Infrared spectral signatures of light r-process elements in kilonovae
- Ce II-IV emission in kilonovae with R-matrix collision strengths and distorted wave recombination rates
- Electron impact excitation of Te IV and V and Level Resolved R-matrix Photoionization of Te I - IV with application to modelling of AT2017gfo
- Lanthanide Impact on the Infra-Red Spectra of Nebular Phase Kilonovae
- Non-LTE analysis for Helium and Strontium lines in the kilonova AT2017gfo
- GWTC-4.0: Population Properties of Merging Compact Binaries
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