Interpreting the main HI and CO l-V features in the Galactic bar from self-consistent stellar and gas dynamical models
classification
🌌 astro-ph
keywords
featuresaccountingcentraldistributiondominantdynamicalgalactichigh
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.