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Application of dynamical system methods to galactic dynamics : from warps to double bars

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Figure 1.1: The main morphological types of galaxies represented by Hubble in the “tuning-fork” diagram.
Figure 1.2: Warped galaxy NGC 5907 and its HI warp as observed by Sancisi (1976) with the Westerbork Synthesis Radio Telescope.
Figure 1.4: Selection of velocity fields of spiral galaxies, assembled by Bosma (1981).
Figure 1.5: Left: Position of the Lagrangian points in a bar potential. Right: Represen- Represen-tative periodic orbits inside the bar.
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