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GRB 250706B/C: Insight-HXMT Discovery of a High-luminosity Burst as a Candidate for Fallback-regulated Accretion in the Prompt Emission

  • Authors: Chen-Wei Wang, R. Moradi, Shao-Lin Xiong, Shuang-Nan Zhang, Zheng-Hang Yu, Wen-Jun Tan, Hao-Xuan Guo, Xiao-Bo Li, Cheng-Kui Li, Jia-Cong Liu, Xing-Hao Luo, Yang-Zhao Ren, Yue Wang, Sheng-Lun Xie, Wang-Chen Xue, Xue-Yuan Zao, Peng Zhang, Chao Zheng

Chen-Wei Wang et al 2026 The Astrophysical Journal Letters 1004 .

  • Provider: AAS Journals

Caption: Figure 1.

The light curve of GRB 250706B/C. (a) The time-resolved spectra and the peak-finding result. (b) The GRB 250706B/C in the T90–MVT diagram. (c) The pulse width of GRB 250706B/C in three different energy ranges (i.e., 60–200 keV, 200–500 keV, and 500–900 keV) as well as the duration of the emission in these three energy ranges. There is no significant broadening or narrowing of both the subpulses and the overall prompt emission as a function of photon energy, suggesting a central-engine-dominated emission process rather than a dissipation-dominated emission process.

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