Discovery of rotation axis alignments in Milky Way globular clusters
Andr\'es E. Piatti

TL;DR
This study reveals a linear relationship between the inclination angles of globular clusters' rotation axes and their orbital axes around the Milky Way, with implications for understanding cluster dynamics and guiding future observations.
Contribution
It uncovers a novel linear correlation between globular clusters' rotation axis inclinations and their orbital inclinations around the Milky Way, independent of other orbital and physical parameters.
Findings
Rotation and orbit axes align at ~56° inclination.
No correlation with orbital size, shape, or internal rotation strength.
Relationship influences future simulations and observational strategies.
Abstract
There is an increasing number of recent observational results which show that some globular clusters exhibit internal rotation while they travel along their orbital trajectories around the Milky Way center. Based on these findings, we looked for any relationship between the inclination angles of the globular clusters' orbits with respect to the Milky Way plane and those of their rotation. We discovered that the relative inclination, in the sense rotation axis inclination - orbit axis inclination, is a function of the globular cluster's orbit inclination. Rotation and orbit axes are aligned for an inclination of ~ 56deg, while the rotation axis inclination is far from the orbit's one between ~ 20deg and -20deg when the latter increases from 0deg up to 90deg. We further investigated the origin of such a linear relationship and found no correlation with the semimajor axes and…
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.
