Dwarf Galaxy Planes: the discovery of symmetric structures in the Local Group
Marcel S. Pawlowski, Pavel Kroupa, Helmut Jerjen

TL;DR
This paper reports the discovery of two symmetric, thin planes of galaxies in the Local Group, revealing a surprising regularity and potential connection between satellite and non-satellite galaxy structures.
Contribution
It introduces the discovery of two symmetric galaxy planes in the Local Group, linking satellite and non-satellite galaxy distributions in a common framework.
Findings
Two symmetric galaxy planes contain nearly all nearby non-satellite galaxies.
The planes are similarly thin, inclined by only 20 degrees to M31's disk.
The planes are connected to known structures like the VPOS and GPoA.
Abstract
Both major galaxies in the Local Group (LG) are surrounded by thin planes of mostly co-orbiting satellite galaxies, the vast polar structure (VPOS) around the Milky Way (MW) and the Great Plane of Andromeda (GPoA) around M31. We summarize the current knowledge concerning these structures and compare their relative orientations and properties in a common coordinate system. The existence of coherent satellite structures motivates an investigation of the distribution of the more distant non-satellite galaxies in the LG. This results in the discovery of two planes (diameters of 1-2 Mpc) which contain almost all nearby non-satellite galaxies. The two LG planes are surprisingly symmetric, inclined by only 20 deg relative to the galactic disc of M31, similarly thin (heights of ~60 kpc) and have near-to-identical offsets from the MW and M31. They are inclined relative to each other by 35 deg.…
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