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Formation of Counterrotating Stellar Disks in the S0 Galaxy PGC 66551

  • Authors: Liuze Long, Min Bao, Qiusheng Gu, Yanmei Chen, Shiying Lu, Yuren Zhou

Liuze Long et al 2026 The Astrophysical Journal 1012 .

  • Provider: AAS Journals

Caption: Figure 4.

(a) and (b) The relative weights and the rotation curves of the main (blue points) and CR (green points) components from I. Y. Katkov et al. (2024). r1 and r2 are the same radius in Figure 1. (c) The rotation curves of CO and Hα. (d) The rotation-velocity difference between CO and Hα versus the radial mean of ﹩\sqrt{{\sigma }_{{\rm{H}}\alpha }^{2}-{\sigma }_{{\rm{C}}{\rm{O}}}^{2}}﹩. The orange and blue points represent the ALMaQUEST kinematic subsample (KSS) and EDGE-CALIFA KSS from Y.-C. Su et al. (2022).

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