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

R. Fux

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

R. Fux

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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.

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R. Fux. 1997-11-03. Interpreting the main HI and CO l-V features in the Galactic bar from self-consistent stellar and gas dynamical models. https://arxiv.org/abs/astro-ph/9711005

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