Gas dynamics in the Galactic bar region

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dc.creatorFux, R.
dc.date1998-11-24
dc.date.accessioned2026-07-07T02:29:15Z
dc.date.available2026-07-07T02:29:15Z
dc.descriptionNew 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.
dc.description2 pages, LaTeX (paspconf.sty), 1 figure. To appear in the proceedings of "Galaxy Dynamics", conference held in Rutgers, August 1998
dc.identifierhttps://arxiv.org/abs/astro-ph/9811384
dc.identifierhttp://arxiv.org/abs/astro-ph/9811384
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13403
dc.subjectAstrophysics
dc.titleGas dynamics in the Galactic bar region
dc.typetext

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