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The Silk Nebula: A Newly Discovered Giant [O III] Emission Filament

  • Authors: Yi-Fei Wu, Song-Yu Jia, Chao-Jian Wu, Chao Zhang, Li-Yue Zhang, Shu Wang, Juan-Juan Ren, Quzhen Dongyang, Hong-Yun Qiu, Zhi-Hong He, Jichen Zhang, Guo-You Sun, Wei-Guo Zhang, Jian-Jun Chen, Hong-Liang Yan, Xiang-Song Fang, Hong Wu

Yi-Fei Wu et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 4.

Relative [O III] intensity distribution map. Plotted points mark the positions where [O III] emission is detected, regions without significant [O III] emission remain blank to avoid the impact of large flux-measurement uncertainties.

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