The Damping and Excitation of Galactic Warps by Dynamical Friction

Details The Damping and Excitation of Galactic Warps by Dynamical Friction The Damping and Excitation of Galactic Warps by Dynamical Friction

1994-08-18

arxiv.org/abs/astro-ph/9408068v1

Astronomy and Astrophysics

Astrophysics

Submitted to MNRAS, 39 pages, uuencoded tar-compressed postscript, CITA-94-33

Scientific paper

We investigate the dynamical interaction of galactic warps with the surrounding dark matter halo, using analytic perturbation theory. A precessing warp induces a density wake in the collisionless dark matter, which acts back on the original warp, transferring energy and angular momentum between the warp and halo (dynamical friction). In most cases dynamical friction damps the warp, but in unusual circumstances (such as a halo that rotates in the same direction as the precession of the warp, or a warp in the equatorial plane of an axisymmetric prolate halo) friction can excite a warp. The damping/excitation time is usually short compared to the Hubble time for realistic systems. Thus most warps cannot be primordial; they must be maintained by some ongoing excitation mechanism.

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