| 5 | | Galaxies can be described in terms of their structure, dynamics |
| 6 | | and stellar populations. Some very robust correlations between |
| 7 | | various galaxy structural properties, such as total luminosity, |
| 8 | | maximum circular velocity, and size have been known for many |
| 9 | | decades yet still lack a theoretical explanation! A fundamental |
| 10 | | challenge to understanding these scaling relations, and ultimately |
| 11 | | galaxy formation and evolution, is the elusive interplay between |
| 12 | | visible and dark matter. I will discuss the latest derivations |
| 13 | | of galaxy scaling relations and our attempts to understand them. |
| | 5 | Galaxies can be described in terms of their structure, dynamics |
| | 6 | and stellar populations. Some very robust correlations between |
| | 7 | various galaxy structural properties, such as total luminosity, |
| | 8 | maximum circular velocity, and size have been known for many |
| | 9 | decades yet still lack a theoretical explanation! A fundamental |
| | 10 | challenge to understanding these scaling relations, and ultimately |
| | 11 | galaxy formation and evolution, is the elusive interplay between |
| | 12 | visible and dark matter. I will discuss the latest derivations |
| | 13 | of galaxy scaling relations and our attempts to understand them. |