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The Coupling of Galactic Dark Matter Halos with Stellar Bars

  • Authors: Angela Collier, and Ann-Marie Madigan

2021 The Astrophysical Journal 915 23.

  • Provider: AAS Journals

Caption: Figure 3.

Time evolution of stellar bar parameters for the three galaxy models. Top: evolution of the bar strength parameter (A2/A0) in the x/y-plane. Middle: evolution of the ratio of the Fourier m = 1 mode to the m = 0 mode (A1z/A0) in the x/z-plane. This quantity represents the growth in asymmetry normal to the midplane. Bottom: evolution of bar pattern speed (Ωb). Models are shown as (blue) circles for the prograde model, (black) diamonds for the nonrotating model, and (red) stars for the retrograde model.

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