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Fast X-Ray Transient EP260321a: Shock Breakout through an Extended Circumstellar Matter

  • Authors: Maokai Hu, Yi Yang, 轶 杨, Xiaofeng Wang

Maokai Hu et al 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure 1.

Schematic illustration of the four evolutionary stages of shock interaction with an extended CSM shell. Stage A: ionization of the CSM by radiation from the SBO at the progenitor’s surface. Stage B: radiative energy accumulation, in which a forward shock propagates through the optically thick CSM and radiation is trapped behind the shock front. Stage C: SBO of the extended CSM while photons diffuse outward through the unshocked CSM. Stage D: cooling phase after the shock has swept up the entire CSM shell.

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