The outer halo globular cluster system of M31 - III. Relationship to the stellar halo
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Authors
Mackey, AD
Ferguson, AMN
Huxor, AP
Veljanoski, J
Lewis, GF
McConnachie, AW
Martin, NF
Ibata, RA
Côté, P
Collins, MLM
Tanvir, NR
Bate, NF
Publication Date
2019-01-01Journal Title
Monthly Notices of the Royal Astronomical Society
ISSN
0035-8711
Publisher
Oxford University Press
Volume
484
Issue
2
Pages
1756-1789
Type
Article
This Version
VoR
Metadata
Show full item recordCitation
Mackey, A., Ferguson, A., Huxor, A., Veljanoski, J., Lewis, G., McConnachie, A., Martin, N., et al. (2019). The outer halo globular cluster system of M31 - III. Relationship to the stellar halo. Monthly Notices of the Royal Astronomical Society, 484 (2), 1756-1789. https://doi.org/10.1093/mnras/stz072
Abstract
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 R proj = 25-150 kpc. In this region the cluster radial density profile exhibits a power-law decline with index = −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 significance. We use our stellar density measurements and previous kinematic data to demonstrate that ≈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 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 R proj = 25 kpc comprises objects accumulated from external galaxies over a Hubble time of growth.
Sponsorship
SCIENCE & TECHNOLOGY FACILITIES COUNCIL (ST/N005805/1)
SCIENCE & TECHNOLOGY FACILITIES COUNCIL (ST/N000927/1)
Identifiers
External DOI: https://doi.org/10.1093/mnras/stz072
This record's URL: https://www.repository.cam.ac.uk/handle/1810/291994
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