http://arxiv.org/abs/2304.13582
Since the mid 70ies it is known that the dwarf galaxies around the Milky Way are arranged in a thin, polar structure. The arrangement and motion within this structure has been identified as a severe challenge to the standard model of cosmology, dubbed as the plane of satellites problem. More observational evidence for such structures has been put forward around other galaxies, such as the Andromeda galaxy, Cen\,A or NGC\,253, among others, adding to the previously identified tensions. Solutions to the plane of satellite problem should therefore not only be tailored to the Milky Way, but need to explain all these different observed systems and environments.
O. Müller
Thu, 27 Apr 23
50/78
Comments: 5 pages. Submitted to the Proceedings of IAU Symposium 379: Dynamical Masses of Local Group Galaxies
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