The formation of galaxies in the CDM Universe: successes and open issues
Oscillatons as Galactic Dark Matter Halos Tonatiuh Matos http:/fis.cinvestav.mx/~tmatos
Problems with the CDM Model
Observational signatures of gas flows toward the center of galaxies Thaisa Storchi Bergmann Instituto de Física, UFRGS, Brazil Collaborators: Barbosa,
Magnetic fields in the Galaxy via Faraday effect: Future prospects with ASKAP and the SKA
Radiation Pressure Supported Starburst Disks & AGN Fueling
Inflation + CDM Model = Cosmology Galaxies Formation
