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H I Depletion Begins Well Beyond the Virial Radius: A FAST Stacking Study of 36 Galaxy Clusters to 5 × R200

  • Authors: Cheng Cheng, Chuan-Peng Zhang, Edo Ibar, Rory Smith, Weiwei Xu, Hyowon Kim, Jia-Sheng Huang, Wei Zhang, Pei Zuo, Hugo Méndez-Hernández, Juan Molina, Ming Zhu, Qian Yu

Cheng Cheng et al 2026 The Astrophysical Journal 1009 .

  • Provider: AAS Journals

Caption: Figure 11.

H I total mass in each clusters within 2R200 (red squares) or 2R200 < R < 5R200 (blue solid dots), in comparison with the simulation results from TNG-Cluster (green diamonds D. Nelson et al. 2024) and TNG300 (coral boxes A. Pillepich et al. 2018; D. Nelson et al. 2018; J. P. Naiman et al. 2018; F. Marinacci et al. 2018; V. Springel et al. 2018). H I abundances from SDSS data from A. Obuljen et al. (2019) are shown in black circles.

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