Skip to content

The outer halo globular cluster system of M31 - III. Relationship to the stellar halo

Research output: Contribution to journalArticle

  • Dougal Mackey
  • Annette Ferguson
  • Avon Huxor
  • Jovan Veljanoski
  • Geraint Lewis
  • Alan McConnachie
  • Rodrigo Ibata
  • Mike Irwin
  • Patrick Côté
  • Michelle Collins
  • Nial Tanvir
  • Nicholas Bate
Original languageEnglish
Pages (from-to)1756–1789
Number of pages34
JournalMonthly Notices of the Royal Astronomical Society
Issue number2
DateAccepted/In press - 24 Dec 2018
DatePublished (current) - 14 Jan 2019


We utilize the final catalogue from the Pan-Andromeda Archaeological Survey to investigate the links between the globular cluster system and field halo in M31 at projected radii Rproj = 25–150 kpc. In this region the cluster radial density profile exhibits a power-law decline with index Γ = −2.37 ± 0.17, matching that for the stellar halo component with [Fe/H] < −1.1. Spatial density maps reveal a striking correspondence between the most luminous substructures in the metal-poor field halo and the positions of many globular clusters. By comparing the density of metal-poor halo stars local to each cluster with the azimuthal distribution at commensurate radius, we reject the possibility of no correlation between clusters and field overdensities at 99.95 per cent 99.95 per cent significance. We use our stellar density measurements and previous kinematic data to demonstrate that ≈35--60 per cent ≈35--60 per cent of clusters exhibit properties consistent with having been accreted into the outskirts of M31 at late times with their parent dwarfs. Conversely, at least ∼40 per cent ∼40 per cent of remote clusters show no evidence for a link with halo substructure. The radial density profile for this subgroup is featureless and closely mirrors that observed for the apparently smooth component of the metal-poor stellar halo. We speculate that these clusters are associated with the smooth halo; if so, their properties appear consistent with a scenario where the smooth halo was built up at early times via the destruction of primitive satellites. In this picture the entire M31 globular cluster system outside Rproj = 25 kpc comprises objects accumulated from external galaxies over a Hubble time of growth.

    Research areas

  • Local Group, globular clusters: general, galaxies: formation, galaxies: haloes, galaxies: individual (M31)

Download statistics

No data available



  • Full-text PDF (final published version)

    Rights statement: This is the final published version of the article (version of record). It first appeared online via University of Oxford Press at Please refer to any applicable terms of use of the publisher.

    Final published version, 21.6 MB, PDF document


View research connections

Related faculties, schools or groups