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A Spatially Resolved H I Survey of Seyfert Galaxies: The Role of Active Galactic Nucleus Feedback in Shaping Atomic Gas Reservoirs

  • Authors: Ruitian Li, Xin Wang, Daizhong Liu, Hui Shi, Yuxuan Pang, Pengfei Ren, Shengzhe Wang, Ming Zhu, Mengting Ju, Xiao-Lei Meng, Xinwen Shu, Ningyu Tang, Jing Wang, Chuan-Peng Zhang, Hong-xin Zhang, Le Zhang, Zheng Zheng, Fujia Li, Chen Xu, Sijia Li, Yiming Yang, Hang Zhou

Ruitian Li et al 2026 The Astrophysical Journal Supplement Series 285 .

  • Provider: AAS Journals

Caption: Figure 3.

Overview of H I kinematic maps for UGC 4503 and UGC 9535. The left panels correspond to UGC 4503 and the right ones display UGC 9535. The H I intensity maps, velocity field maps, and velocity dispersion maps are presented from top to bottom, respectively. The white and black contours mark H I spatial distribution boundaries of our targets, which are defined when H I surface densities reach 1 M⊙ pc−2 (J. Wang et al. 2016).

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