Interpreting the main HI and CO l-V features in the Galactic bar from self-consistent stellar and gas dynamical models
| dc.creator | Fux, R. | |
| dc.date | 1997-11-03 | |
| dc.date.accessioned | 2026-07-07T02:24:53Z | |
| dc.date.available | 2026-07-07T02:24:53Z | |
| dc.description | 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. | |
| dc.description | 2 pages, LaTeX, 1 figure. To appear in Proc. IAU Symp. 184, "The Central Regions of the Galaxy and Galaxies", ed. Y. Sofue. Part of Fux 1997, PhD thesis, Geneva Observatory. Also available at http://obswww.unige.ch/Preprints/cgi-bin/Preprintshtml.cgi?#DYNAMIC | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9711005 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9711005 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11729 | |
| dc.subject | Astrophysics | |
| dc.title | Interpreting the main HI and CO l-V features in the Galactic bar from self-consistent stellar and gas dynamical models | |
| dc.type | text |