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astro-ph.HE2026
A temporally clustered gravitational wave pair and a Type IIb supernova
Sheng Yang, Ting-Wan Chen, Weichangfeng Guo +22
Compact object mergers are generally expected long after the stellar collapse that forms their remnants. Here we report two marginal gravitational wave (GW) candidates, S190910d an…
astro-ph.HE2026
Constraining the Pulsar 3D Velocity Distribution: The Impact of Spin-Velocity Alignment
Zheng Li, Xiaojin Liu, Zhi-Qiang You +2
Quantifying the natal kick distribution of pulsars is essential for understanding supernova physics and binary evolution, yet measurements are historically limited by the lack of r…