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Pinning Down the Geometry of the Type Ic Broad-line Supernova 2026gzf

  • Authors: Xudong Wen, 旭东 文, Yi Yang, 轶 杨, Jing Lu, 晶 陆, Lifan Wang, J. Craig Wheeler, Miika Pursiainen, QiuJu Huang, Bao Wang, Xuefeng Wu, Alexei V. Filippenko, Wolfgang E. Kerzendorf, Giorgos Leloudas, Steve Schulze, Ferdinando Patat

Xudong Wen et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure A2.

Predicted continuum polarization from MCPOL simulations for axisymmetric ellipsoidal ejecta with different axial ratios and electron-scattering optical depths. Panel (A) shows the continuum polarization as a function of viewing angle for axial ratios A = 1.05, 1.1, 1.2, and 1.3. Blue and red curves correspond to photons emitted from electron-scattering optical depths of τ = 1 and τ = 3, respectively. The horizontal dashed line marks the observed bias-corrected continuum polarization, while the shaded region indicates its uncertainty. Panel (B) shows the continuum polarization as a function of electron-scattering optical depth for viewing angles of 30, 60, and 90. Colors denote different axial ratios, while line styles represent different viewing angles.

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