Kinematics and Metallicity of Red Giant Branch Stars in the Northeast Shelf of M31
Ivanna Escala, Karoline M. Gilbert, Mark Fardal, Puragra Guhathakurta,, Robyn E. Sanderson, Jason S. Kalirai, Bahram Mobasher

TL;DR
This study uses spectroscopic data of red giant stars in M31's Northeast shelf to detect a wedge velocity pattern, supporting models of tidal debris formation from a radial merger and revealing the metallicity distribution of the tidal material.
Contribution
First detection of a complete wedge pattern in M31's NE shelf, providing strong evidence for tidal shell formation from a radial merger and confirming the association of multiple tidal features.
Findings
Detected a wedge pattern consistent with a tidal shell model.
Found the metallicity distribution matches that of the Giant Stellar Stream.
No kinematic signature of an intact progenitor core was observed.
Abstract
We obtained Keck/DEIMOS spectra of 556 individual red giant branch stars in 4 spectroscopic fields spanning projected kpc along the Northeast (NE) shelf of M31. We present the first detection of a complete wedge pattern in the space of projected M31-centric radial distance versus line-of-sight velocity for this feature, which includes the returning stream component of the shelf. This wedge pattern agrees with expectations of a tidal shell formed in a radial merger and provides strong evidence in favor of predictions of Giant Stellar Stream (GSS) formation models in which the NE shelf originates from the second orbital wrap of the tidal debris. The observed concentric wedge patterns of the NE, West (W), and Southeast (SE) shelves corroborate this interpretation independently of the models. We do not detect a kinematical signature in the NE shelf region corresponding to an intact…
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