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On the Role of Noncircular Motions in MaNGA Galaxies. I. Global Properties

  • Authors: Carlos López-Cobá, Lihwai Lin, Justus Neumann, Matthew A. Bershady

Carlos López-Cobá et al 2024 The Astrophysical Journal 975 .

  • Provider: AAS Journals

Caption: Figure 5.

Comparison between maximum rotational velocities estimated from the circular rotation velocities V t (r), and the c 1(r) velocities from the harmonic model. Every point here represents one individual object. The black straight line represents the 1-to-1 line. The inset panel shows a violin plot of the difference between both velocities, i.e., ﹩{\rm{\Delta }}V={V}_{\max ,c1}-{V}_{\max ,t}﹩. The dispersion of the difference is 5 km s−1.

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