Is M31 at the center of its satellite system ?
Amandine Doliva-Dolinsky, N. F. Martin, Michelle L. M. Collins

TL;DR
This study investigates whether M31 is at the center of its satellite galaxy distribution, finding a possible slight offset but not statistically significant, emphasizing the need for more satellite discoveries to clarify the structure.
Contribution
The paper introduces a forward modeling approach that accounts for search completeness to assess M31's satellite distribution center relative to M31 itself.
Findings
Displacement of 10-50 kpc towards the Milky Way from M31's center.
Offset significance ranges from ≤1σ to 1.9σ, depending on assumptions.
Quadrupling known satellites could reveal a significant offset.
Abstract
The arrangement of M31's dwarf galaxies exhibits anisotropy, with the majority located in the hemisphere between the Milky Way and the host galaxy. This study aims to investigate whether M31's present location is aligned with the center of its distribution of dwarf galaxies. We use forward modeling to infer the center of the M31 satellite 3D spatial distribution, folding in the completeness of dwarf galaxy searches. We observe a displacement of the center of the satellite distribution, relative to the center of M31, of approximately 10--50 kpc towards the Milky Way. Nonetheless, the center of M31 remains compatible with the center of the dwarf galaxy distribution given the broad constraints on its position, with the significance of the shift ranging from to , depending on the assumed form of the volumetric spatial distribution of satellites. If M31 is truly…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies
