Changes between Version 3 and Version 4 of Talks/Fall2006/Colloquium/061115
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- 10/15/06 12:43:04 (19 years ago)
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Talks/Fall2006/Colloquium/061115
v3 v4 17 17 ''Secular Evolution of Galaxies: From Dark Halos to Nuclei''[[BR]] 18 18 19 {{One path by which disk galaxies evolve is via internal secular[[BR]]19 One path by which disk galaxies evolve is via internal secular[[BR]] 20 20 evolution. By breaking the symmetry of the system, bars play an[[BR]] 21 21 important role in driving such evolution. I describe some recent[[BR]] 22 22 results concerning aspects of this evolution relating to dark halos, disk[[BR]] 23 density profiles, bulges and central nuclei. }}23 density profiles, bulges and central nuclei.
