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

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

1997-11-03

arxiv.org/abs/astro-ph/9711005v1

Astronomy and Astrophysics

Astrophysics

2 pages, LaTeX, 1 figure. To appear in Proc. IAU Symp. 184, "The Central Regions of the Galaxy and Galaxies", ed. Y. Sofue. Pa

Scientific paper

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.

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