Astr 328 Jan 29, 2003: The distance scale
Virgo cluster velocity
Measuring cluster velocity with
different galaxy types
Discussion question
Virgocentric flow
Measuring H0 using Virgo
Using a better cluster: Fornax
Why Fornax is a better cluster
Averaging over local groups of galaxies
H0 plot from local galaxies
Go further out....
A word from the opposition
Secondary distance indicators
Surface brightness fluctuations
Illustrate with extreme case
As galaxies become more distant,
their light gets smoother
Poisson distribution
Observational complications
SBF is for elliptical galaxies, not spirals
Metal-poor globular CMD
Metal-rich globular CMD
Globular cluster luminosity function
And its many problems