Image Details

Choose export citation format:

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 2.

Afterglow light curves in the X-ray (5 keV; orange), near-infrared (2 × 1014 Hz; blue), and radio (1.3 GHz; red) bands, compared with the observed data of GRB 250702B (X-ray: orange circles; near-infrared: blue diamonds; radio: red squares). The thick solid and thin dashed lines denote the predicted emission for the maximum (40 jets) and minimum (four jets) cases, respectively. Black arrows indicate the times of the observed gamma-ray flares.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse