Gas dynamics in the Galactic bar region

Astronomy and Astrophysics – Astrophysics

Scientific paper

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2 pages, LaTeX (paspconf.sty), 1 figure. To appear in the proceedings of "Galaxy Dynamics", conference held in Rutgers, August

Scientific paper

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.

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