2 papers
astro-ph.SR2026
Quantifying Element Importance for Mass Recovery from Population III Supernova Yield Fits
Zhongyuan Zhang, Alexander P Ji, Vinicius M Placco +1
Massive Population III stars are currently not observed, but their initial mass function (IMF) can be inferred through stellar archaeology: fitting core-collapse supernova yield mo…
astro-ph.HE2025
2D End-to-End Modeling of Kilonovae from Binary Neutron Star Merger Remnants
Lieke Sippens Groenewegen, Sanjana Curtis, Philipp Mösta +2
We investigate the kilonova emission resulting from outflows produced in a three-dimensional (3D) general-relativistic magnetohydrodynamic (GRMHD) simulation of a hypermassive neut…