The faint globular cluster in the dwarf galaxy Andromeda I
  Observations of globular clusters in dwarf galaxies can be used to study a
variety of topics, including the structure of dark matter halos and the history
of vigorous star formation in low-mass galaxies. We report on the properties of
the faint globular cluster (M_V ~ -3.4) in the M31 dwarf galaxy Andromeda I.
This object adds to the growing population of low-luminosity Local Group
galaxies that host single globular clusters.
