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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 10.

First panel: simulated axisymmetric velocity field plus random noise; the disk is inclined at i = 35° and is oriented at ﹩{\phi }_{\mathrm{disk}}^{{\prime} }=77^\circ ﹩; the rotation curve adopted follows Equation (3), with V 0 = 170 km s−1 and r t = 2″. Middle panel: model recovered using XS. Third panel: residual map, namely observed – model. Fourth panel: cumulative distribution of the residual velocities. Different percentiles are highlighted, going from 10% (V 10) to 90% (V 90). 1σ encloses 84% of the data, while ﹩{V}_{80}=({V}_{90}-{V}_{10})/\sin i﹩. The ratio V 80/σ = 2.67, which is approximately 1.1 FWHM.

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