1998/11/24 by R. Fux, Fux, R.
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #Astrophysics and Star Formation Studies #FOS: Physical sciences #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9811384
2 pages, LaTeX (paspconf.sty), 1 figure. To appear in the proceedings of "Galaxy Dynamics", conference held in Rutgers, August 1998
arxiv created 1998/11/24 · openalex publication_date 1998/11/24 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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.