Spiral and Bar Instabilities Provoked by Dark Matter Satellites

Details Spiral and Bar Instabilities Provoked by Dark Matter Satellites Spiral and Bar Instabilities Provoked by Dark Matter Satellites

2008-02-27

arxiv.org/abs/0802.3997v1

Astronomy and Astrophysics

Astrophysics

4 pages, 1 figure, 4 movies at http://www.cita.utoronto.ca/~dubinski/Rome2007, to appear in the proceedings of the ASP, Form

Scientific paper

We explore the secular dynamical evolution of an N-body model of M31 in the presence of a population of 100 dark matter satellites over 10 Gyr. The satellite population has structural and kinematic characteristics modelled to follow the predictions of Lambda-CDM cosmological simulations. Vertical disk heating is a small effect despite many interactions with the satellite population with only a 20% increase in vertical velocity dispersion sigma_z and the disk scale height z_d at the equivalent solar radius R = 2.5R_d . However, the stellar disk is noticeably flared after 10 Gyr with z_d nearly doubling at the disk edge. Azimuthal disk heating is much larger with sigma_R and sigma_z both increasing by 1.7x. However, in a control experiment without satellites dispersion increases by 1.5x suggesting that most of the effect is due to heating through scattering off of spiral structure excited by swing-amplified noise. Surprisingly, direct impacts of satellites on the disk can excite spiral structure with a significant amplitude and in some cases impacts close to the disk center also induce the bar instability. The large number of dark matter satellite impacts expected over a galaxy's lifetime may be a significant source of external perturbations for driving disk secular evolution.

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