| 15 | | 'One path by which disk galaxies evolve is via internal secular |
| 16 | | evolution. By breaking the symmetry of the system, bars play an |
| 17 | | important role in driving such evolution. I describe some recent |
| 18 | | results concerning aspects of this evolution relating to dark halos, disk |
| 19 | | density profiles, bulges and central nuclei.' |
| | 17 | ''Secular Evolution of Galaxies: From Dark Halos to Nuclei''[[BR]] |
| | 18 | |
| | 19 | {{One path by which disk galaxies evolve is via internal secular[[BR]] |
| | 20 | evolution. By breaking the symmetry of the system, bars play an[[BR]] |
| | 21 | important role in driving such evolution. I describe some recent[[BR]] |
| | 22 | results concerning aspects of this evolution relating to dark halos, disk[[BR]] |
| | 23 | density profiles, bulges and central nuclei.}} |