Spiral Structure Dynamics in Pure Stellar Disk Models
arXiv:1310.4674
Abstract
In order to understand the physical mechanism underlying non-steady stellar spiral arms in disk galaxies we performed a series of N-body simulations with 1.2 and 8 million particles. The initial conditions were chosen to follow Kuijken-Dubinski models. In this work we present the results of a sub-sample of our simulations in which we experiment with different disk central radial velocity dispersion and the disk scale height.
To appear in the conference proceedings of "Structure and Dynamics of Disk Galaxies", M.S. Seigar and P. Treuthardt, eds