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Andreoni , I · 2024

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astro-ph.HE 1

years

2025 1

verdicts

CONDITIONAL 1

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Inferring neutron star merger ejecta morphologies with kilonovae

astro-ph.HE · 2025-05-22 · conditional · novelty 6.0

Kilonova ejecta morphology is distinguishable only when late-time JWST mid-infrared data are added to Rubin optical data, and AT2017gfo is best matched by the SuperNu TP2 (toroidal plus peanut wind) model.

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  • Inferring neutron star merger ejecta morphologies with kilonovae astro-ph.HE · 2025-05-22 · conditional · none · ref 4

    Kilonova ejecta morphology is distinguishable only when late-time JWST mid-infrared data are added to Rubin optical data, and AT2017gfo is best matched by the SuperNu TP2 (toroidal plus peanut wind) model.