An intriguing coincidence between the majority of vast polar structure dwarfs and a recent major merger at the M31 position
Istiak Akib, Fran\c{c}ois Hammer, Yanbin Yang, Marcel S. Pawlowski,, Jianling Wang

TL;DR
This study explores a potential link between the Vast Polar Structure of the Milky Way's dwarf galaxies and a major merger event in Andromeda, suggesting a shared origin through tidal interactions and matter exchange.
Contribution
It provides evidence for a possible association between M31 tidal tails and MW dwarf galaxies, offering a new explanation for the origin of the VPOS.
Findings
Potential association between M31 tidal tails and MW dwarfs in 6D phase space.
Low-mass MW models show dwarf galaxies can be linked to M31 tidal features.
Ram pressure effects could have slowed dwarf galaxy motions, supporting the association.
Abstract
A significant part of the Milky Way (MW) dwarf galaxies orbit within a Vast POlar Structure (VPOS), which is perpendicular to the Galactic disc and whose origin has not yet been identified. It includes the Large Magellanic Cloud (LMC) and its six dynamically associated dwarf galaxies. Andromeda Galaxy (M31) experienced a major merger two to three billion years ago, and its accurate modelling predicts that an associated tidal tail is pointing towards the Galaxy. Here, we tested a possible association between M31 tidal tail particles and MW dwarf galaxies, focusing first on the LMC and its associated dwarfs since they are less affected by ram pressure. We traced back these dwarf galaxy orbits by one billion years and calculated their association with the tidal tail particles in the 6D phase space, based on their proper motion from \textit{Gaia} DR3. We find that for low-mass MW models…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysical Phenomena and Observations · Astronomy and Astrophysical Research
