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Successive Partial Disruptions with Orbital Precession in a White Dwarf–Black Hole System for Repeating GRB 250702B

  • Authors: Yuri Sato, Rin Oikawa, Kazuma Kato, Tatsuya Matsumoto, Kazumi Kashiyama

Yuri Sato et al 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure 3.

Predicted radio (1.3 GHz) afterglow light curves for the maximum (40 jets; red solid line) and minimum (four jets; red dashed line) cases. The gray solid lines show the emission from individual jets in the maximum case, while the black dashed lines represent the emission from individual jets in the minimum case. At T ∼ 108 s, the maximum case is approximately an order of magnitude brighter than the minimum case.

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