Cambridge University Press (CUP), Publications of the Astronomical Society of Australia, (34), 2017
DOI: 10.1017/pasa.2017.35
Full text: Unavailable
AbstractObservations 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 (MV ~ −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.