The Vast Polar Structure of the Milky Way and Filamentary Accretion of Sub-Halos
Marcel S. Pawlowski

TL;DR
The paper investigates the origin of the Milky Way's vast polar structure of satellites, finding that filamentary accretion models cannot explain the observed correlations, and suggesting tidal dwarf galaxies as a plausible alternative formation scenario.
Contribution
It challenges the filamentary accretion hypothesis for the Milky Way's satellite distribution and proposes tidal dwarf galaxies as a natural formation explanation.
Findings
Filamentary accretion models fail to reproduce satellite orbit correlations.
High-resolution simulations do not support filamentary origin of the VPOS.
Tidal dwarf galaxies offer a plausible alternative formation scenario.
Abstract
The Milky Way (MW) is surrounded by numerous satellite objects: dwarf galaxies, globular clusters and streams of disrupted systems. Together, these form a vast polar structure (VPOS), a thin plane spreading to Galactocentric distances as large as 250 kpc. The orbital directions of satellite galaxies and the preferred alignment of streams with the VPOS demonstrate that the objects orbit within the structure. This strong phase-space correlation is at odds with the expectations from simulations of structure formation based on the cold dark matter cosmology (LCDM). The accretion of sub-halos along filaments has been suggested as the origin of the anisotropic distribution. We have tested this scenario using the results of high-resolution cosmological simulations and found it unable to account for the large degree of correlation of the MW satellite orbits. It is therefore advisable to search…
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