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The Shapes of the H I Velocity Profiles of the THINGS Galaxies

  • Authors: R. Ianjamasimanana, W. J. G. de Blok, Fabian Walter, and George H. Heald

Ianjamasimanana et al. 2012 The Astronomical Journal 144 96.

  • Provider: AAS Journals

Caption: Figure 4.

Super profile parameters derived from the model data cubes of IC 2574 and NGC 2403 as a function of the resolution. Solid and open symbols represent the models of IC 2574 and NGC 2403, respectively. The circle symbols represent the 63° models, whereas the star symbols represent the 80° inclination models. We only present the single Gaussian fitting results of the IC 2574 models as these profiles do not show a double Gaussian function signature. Left panel: single Gaussian velocity dispersion. Middle panel: narrow component velocity dispersion. Right panel: broad component velocity dispersion.

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