Interpreting the main HI and CO l-V features in the Galactic bar from self-consistent stellar and gas dynamical models
Astrophysics
2007-05-23 v1
Abstract
A new picture accounting for the dominant features in the observed l-V distribution of the Milky Way gas within the central few kpcs is proposed, based on symmetry-free and high resolution 3D N-body and SPH simulations.
Cite
@article{arxiv.astro-ph/9711005,
title = {Interpreting the main HI and CO l-V features in the Galactic bar from self-consistent stellar and gas dynamical models},
author = {R. Fux},
journal= {arXiv preprint arXiv:astro-ph/9711005},
year = {2007}
}
Comments
2 pages, LaTeX, 1 figure. To appear in Proc. IAU Symp. 184, "The Central Regions of the Galaxy and Galaxies", ed. Y. Sofue. Part of Fux 1997, PhD thesis, Geneva Observatory. Also available at http://obswww.unige.ch/Preprints/cgi-bin/Preprintshtml.cgi?#DYNAMIC