The rotationally stabilized VPOS and predicted proper motions of the Milky Way satellite galaxies
Marcel S. Pawlowski, Pavel Kroupa

TL;DR
The paper demonstrates that the Milky Way's satellite galaxies form a rotationally stabilized structure called the VPOS, and uses this to predict their proper motions, challenging standard cosmological models.
Contribution
It provides empirical predictions of satellite proper motions based on the VPOS's rotational stability, supporting tidal dwarf galaxy origins over dark matter models.
Findings
Most satellites have aligned orbital poles, indicating a rotationally stabilized VPOS.
Predicted proper motions match well with existing measurements, validating the method.
Satellite velocities suggest an effective gravitational potential with a constant velocity of ~240 km/s.
Abstract
The satellite galaxies of the Milky Way (MW) define a vast polar structure (VPOS), a thin plane perpendicular to the MW disc. Proper motion (PM) measurements are now available for all of the 11 brightest, `classical' satellites and allow an updated analysis of the alignment of their orbital poles with this spatial structure. The coherent orbital alignment of 7 to 9 out of 11 satellites demonstrates that the VPOS is a rotationally stabilized structure and not only a pressure-supported, flattened ellipsoid. This allows us to empirically and model independently predict the PMs of almost all satellite galaxies by assuming that the MW satellite galaxies orbit within the VPOS. As a test of our method, the predictions are best met by satellites whose PMs are already well constrained, as expected because more uncertain measurements tend to deviate more from the true values. Improved and new PM…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
