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Dwarf galaxies

Planes of satellites no longer in tension with ΛCDM

The arrangement of dwarf galaxies in a thin plane surrounding the Milky Way has been thought to contradict the prevailing cosmological model of cold dark matter in the Universe. New work suggests that this arrangement may just be a temporary alignment, bringing our galaxy back into agreement with theoretical expectations once the radial distribution of satellites is taken into account.

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Fig. 1: The unusual thinness of the plane of satellites in the Milky Way is heavily defined by two of the most distant satellites, Leo I and Leo II.

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Correspondence to Laura V. Sales.

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Sales, L.V., Navarro, J.F. Planes of satellites no longer in tension with ΛCDM. Nat Astron 7, 376–377 (2023). https://doi.org/10.1038/s41550-023-01924-y

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