Milky Way Gas Dynamics

Details Milky Way Gas Dynamics Milky Way Gas Dynamics

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005dda....36.1401e&link_type=abstract

American Astronomical Society, DDA meeting #36, #14.01; Bulletin of the American Astronomical Society, Vol. 37, p.533

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The Milky Way is made up of a central bar, a disk with embedded spiral arms, and a dark matter halo. Observational and theoretical constraints for the characteristic parameters of these components will be presented, with particular emphasis on the constraints from the dynamics of the Milky Way gas. In particular, the fraction of dark matter inside the solar radius, the location of the main resonances, and the evidence for multiple pattern speeds will be discussed.

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