Interpreting the main HI and CO l-V features in the Galactic bar from self-consistent stellar and gas dynamical models
Abstract
Description
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.
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
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