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Microquasar Cygnus X-3 as the PeVatron Powering the Cygnus Bubble

  • Authors: Zhaodong Shi, Guangwei Wang, Rui-zhi Yang, Felix Aharonian

Zhaodong Shi et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 3.

Same as Figure 1, but the right panel displays the azimuthally averaged integrated γ-ray intensity above 400 TeV, and the gas distribution is nonhomogeneous and is given by Equation (12) with n0 = 1 cm−3 and zc = 300 pc, while the CR injection kinetic powers are given in Table 2.

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