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Fast X-Ray Transients from Dense Circumstellar Material Shock Breakout and Cooling Emission

  • Authors: Jin-Ping Zhu, Yi-Han Iris Yin, Yun-Wei Yu, Zhuo Li, Bing Zhang

Jin-Ping Zhu et al 2026 The Astrophysical Journal Letters 1012 .

  • Provider: AAS Journals

Caption: Figure 5.

Simulated observed lightcurves and spectral peak temperature evolution of SN SBO and subsequent cooling emission in dense CSM shell for different rout (top left), χ (top right), MCSM (bottom left), and vsh (bottom right). In each panel, the upper subpanel presents the observed lightcurves in both the bolometric band (solid lines) and soft X-ray band (dashed lines; 0.5–4 keV), while the lower subpanel shows the evolution of the observed spectral peak temperature. Each panel shows four choices of the corresponding parameter, including the fiducial values of rout = 3.2 × 102 R⊙, χ = 0.1, MCSM = 3.2 × 10−4 M⊙, and vsh = 0.15c.

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