A wind-reprocessing model of unstable mass transfer onto neutron stars and black holes is fit to the long-rising precursors of SN 2023zkd, SN 2023fyq, and SN 2021qqp, inferring mass-loss histories consistent with binary merger progenitors.
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Semi-analytical Light Curve Model for Transients Preceding Binary Mergers. I: Supernova Precursor Emission from Compact Object Companions
A wind-reprocessing model of unstable mass transfer onto neutron stars and black holes is fit to the long-rising precursors of SN 2023zkd, SN 2023fyq, and SN 2021qqp, inferring mass-loss histories consistent with binary merger progenitors.