Abstract
We utilise 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 $R_p=25-150$ kpc. In this region the cluster radial density profile exhibits a power-law decline with index $\Gamma=-2.37\pm0.17$, matching that for the stellar halo component with [Fe/H] $
Original language | English |
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Pages (from-to) | 1756–1789 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 484 |
Issue number | 2 |
DOIs | |
Publication status | Published - 14 Jan 2019 |
Keywords
- astro-ph.GA