The nature of the Eastern Extent in the outer halo of M31
Janet Preston, Michelle Collins, R. Michael Rich, Rodrigo Ibata,, Nicolas F. Martin, Mark Fardal

TL;DR
This study provides the first detailed spectroscopic analysis of the Eastern Extent in M31's outer halo, revealing its properties and potential connection to the Giant Stellar Stream through kinematics and metallicity measurements.
Contribution
It offers new spectroscopic data and analysis of the Eastern Extent, suggesting its possible origin from the progenitor of the Giant Stellar Stream and linking multiple halo substructures.
Findings
Eastern Extent has systemic velocities between -368 km/s and -331 km/s.
Photometric metallicities are metal-poor, around -0.9 on average.
Properties of the Eastern Extent are consistent with those of the Giant Stellar Stream.
Abstract
We present the first comprehensive spectroscopic study of the Andromeda galaxy's Eastern Extent. This ~4 degree long filamentary structure. located 70-90 kpc from the centre of M31, lies perpendicular to Andromeda's minor axis and the Giant Stellar Stream and overlaps Stream C. In this work, we explore the properties of the Eastern Extent to look for possible connections between it, the Giant Stellar Stream and Stream C. We present the kinematics and photometry for ~50 red giant branch stars in 7 fields along the Eastern Extent. We measure the systemic velocities for these fields and find them to be -368 km/s < v < -331 km/s with a slight velocity gradient of -0.51 +/- 0.21 km/s/kpc towards the Giant Stellar Stream. We derive the photometric metallicities for stars in the Eastern Extent finding them to be metal-poor with values of -1.0 < [Fe/H]phot < -0.7 with a <[Fe/H]phot> ~-0.9. We…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
