Gas dynamics in the Galactic bar region from N-body and SPH simulations
Abstract
Self-consistent hybrid N-body and SPH simulations are used to give a new and coherent interpretation of the main features standing out from the HI and CO longitude-velocity observations within the Galactic bar. In particular, the traces of the gas associated to the Milky Way's dustlanes can be reliably identified and the 3-kpc arm appears as a gaseous stream rather than a density wave. The bar and the gaseous nuclear ring in the simulations undergo synchronised and long lived oscillations around the centre of mass, and the gas flow always remains non-stationary, suggesting a transient nature of the observed gas kinematics.
Cite
@article{arxiv.astro-ph/9908091,
title = {Gas dynamics in the Galactic bar region from N-body and SPH simulations},
author = {R. Fux},
journal= {arXiv preprint arXiv:astro-ph/9908091},
year = {2009}
}
Comments
8 pages, 4 figures. To appear in the proceedings of "The Evolution of Galaxies on Cosmological Timescales", eds. J.E. Beckman and T. Mahoney, Astrophysics and Space Science