Gas dynamics in the Galactic bar region
Abstract
Description
New constraints on the Milky Way's bar parameters are derived from the gaseous spiral structure within the Galactic bar, and in particular from the identification of the dustlanes leading the bar major axis.
2 pages, LaTeX (paspconf.sty), 1 figure. To appear in the proceedings of "Galaxy Dynamics", conference held in Rutgers, August 1998
2 pages, LaTeX (paspconf.sty), 1 figure. To appear in the proceedings of "Galaxy Dynamics", conference held in Rutgers, August 1998