The faint globular cluster in the dwarf galaxy Andromeda I
Astrophysics of Galaxies
2017-09-13 v1
Abstract
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.
Cite
@article{arxiv.1708.03596,
title = {The faint globular cluster in the dwarf galaxy Andromeda I},
author = {Nelson Caldwell and Jay Strader and David J. Sand and Anil C. Seth and Beth Willman},
journal= {arXiv preprint arXiv:1708.03596},
year = {2017}
}
Comments
PASA in press