IMF
Microlensing
White dwarf cooling track
Beige dwarfs, or is it acru?
Summary
Dwarf Spheroidal galaxies
Sculptor dSph galaxy
Radial Velocities
large Velocity dispersion
King models
Tidal disruption
dSph galaxies, tidal disruption and light profiles
dSph magnified
Velocity Vectors
dynamics of tidal disruption
Question: Can you think of a scenario?
dSph summary
Question: Why was this so hard?
Local Group dSph galaxies
Velocity dispersion and probablility graphs
