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Warped Disk Galaxies: Alignment with the Large-scale Tidal Field

  • Authors: Yiheng Wang, Huiyuan Wang, Enci Wang, Xi Kang

Yiheng Wang et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 3.

Distribution of ﹩| \cos \theta | ﹩ between the galaxy major axis and the tidal field t1 direction for central galaxies in two stellar mass bins, using warped galaxies and a matched nonwarped control sample. The left and right panels correspond to ﹩8\leqslant \mathrm{log}({M}_{\star }/{M}_{\odot })\lt 10﹩ and ﹩10\leqslant \mathrm{log}({M}_{\star }/{M}_{\odot })\lt 11.5﹩, respectively. The curves show probability density functions (PDFs) computed from the data normalized relative to a uniform distribution. The shaded regions represent 1σ uncertainties estimated via bootstrap resampling (Nboot = 2000).

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