Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 8.

Left and middle panels: SNR diagnostic model from L. Sabin et al. (2013), where green points mark locations on the [O III] structure and gray points mark the background. The orange circle marks the distribution of DIG regions in the BPT diagrams. Right panel: 2D diagnostic model proposed by M. Kopsacheili et al. (2020), with red points indicating data located on the [O III] structure.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse