Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-25T15:48:50.284Z Has data issue: false hasContentIssue false

Properties of the Galactic Bar from Hydrodynamical Simulations

Published online by Cambridge University Press:  25 May 2016

Benjamin J. Weiner
Affiliation:
Dept. of Physics and Astronomy, Rutgers University P.O. Box 849, Piscataway, NJ 08855, USA
J.A. Sellwood
Affiliation:
Dept. of Physics and Astronomy, Rutgers University P.O. Box 849, Piscataway, NJ 08855, USA

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

It is well known that the existence of H I and CO gas at “forbidden” velocities in longitude-velocity (l–V) diagrams of the inner Galaxy (e.g. Liszt & Burton 1980, Liszt 1992) is inconsistent with circular motion in an axisymmetric potential. Gas flow in a barred potential could be consistent with the observations, however. We have compared the observations to 2-D hydrodynamical simulations of gas flows in a family of barred potentials. The gas flow pattern is very sensitive to the assumed potential, and the l–V distribution of cool gas in the inner Galaxy places strong constraints on several parameters of the Milky Way bar.

Type
Chapter 2: Is the Milky Way a Barred Spiral Galaxy?
Copyright
Copyright © Kluwer 1996 

References

Athanassoula, E. 1992, MNRAS 259, 345.Google Scholar
Liszt, H.S. 1992, in The Center, Bulge, and Disk of the Milky Way , ed. Blitz, L., (Dordrecht: Kluwer), p. 111.CrossRefGoogle Scholar
Liszt, H.S., & Burton, W.B. 1980, Ap. J. 236, 779.Google Scholar
van Albada, G.D. 1985, in The Milky Way Galaxy, IAU Symp. 106 , ed. van Woerden, H. et al. (Dordrecht: Kluwer), p.547.Google Scholar