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Photoionization of the Composite Nebula Surrounding NGC 5408 X-1: Implications for Beamed Emission

  • Authors: Jing Guo, 静 郭, Hua Feng, Roberto Soria, Fuyan Bian, Jianfeng Wu, Lian Tao, Jesús M. Corral-Santana

Jing Guo et al 2026 The Astrophysical Journal 1010 .

  • Provider: AAS Journals

Caption: Figure 6.

Radial emissivity profiles predicted by CLOUDY with the dual-component model. The dashed line marks the peak [O III] λ5007 emissivity position (∼18 pc), matching the observed peak displacement (see Figure 1).

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