Dynamical Friction in Barred Galaxies

Details Dynamical Friction in Barred Galaxies Dynamical Friction in Barred Galaxies

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...189.5403d&link_type=abstract

American Astronomical Society, 189th AAS Meeting, #54.03; Bulletin of the American Astronomical Society, Vol. 28, p.1344

Astronomy and Astrophysics

Astronomy

Scientific paper

Observations of barred galaxies suggest that bars are in rapid rotation.
Simulations show that in the presence of a massive halo, dynamical
friction quickly slows down the bar. This problem is not present if the
galaxy has a less massive halo, similar to a maximum disk model.

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