| Issue |
A&A
Volume 706, February 2026
|
|
|---|---|---|
| Article Number | A193 | |
| Number of page(s) | 16 | |
| Section | Galactic structure, stellar clusters and populations | |
| DOI | https://doi.org/10.1051/0004-6361/202557613 | |
| Published online | 12 February 2026 | |
A vertically orientated dark matter halo marks a flip of the Galactic disc
1
Shanghai Astronomical Observatory, Chinese Academy of Sciences,
80 Nandan Road,
Shanghai
200030,
China
2
Institute for Astronomy the School of Physics, Zhejiang University,
38 Zheda Road,
Hangzhou,
310027
Zhejiang,
China
3
National Astronomical Observatories, Chinese Academy of Sciences,
Beijing
100101,
China
4
School of Physics and Optoelectronic Engineering, Hainan University,
58 Renmin Avenue,
Haikou
570228,
China
5
Department of Astronomy, Westlake University,
Hangzhou,
Zhejiang
310030,
China
6
Institute for Frontiers in Astronomy and Astrophysics, Beijing Normal University,
Beijing
102206,
China
★ Corresponding authors: This email address is being protected from spambots. You need JavaScript enabled to view it.
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Received:
9
October
2025
Accepted:
25
November
2025
Unveiling the 3D shape of the Milky Way’s dark-matter halo is critical to understanding its formation history. We created an innovative dynamical model that makes minimal assumptions about the internal dynamical structures and accommodates a highly flexible triaxial DM halo. By applying the method to 6D phase-space data of K-giant stars from LAMOST + Gaia, we robustly determined the 3D dark-matter distribution of the Milky Way out to approximately 50 kpc. We discovered a triaxial, nearly oblate dark-matter halo with qDM = Z/X = 0.92 ± 0.08, pDM = Y/X = 0.8 ± 0.2 on average within 50 kpc, where the Z-axis is defined perpendicular to the stellar disc. The axes ratio qDM > pDM is strongly preferred; the long-intermediate axis plane of the dark-matter halo is unexpectedly vertical to the Galactic disc, yet aligned with the ‘plane of satellites’. This striking configuration suggests that the Galactic disc (and the inner halo) has flipped, likely torqued by minor mergers, from an original alignment with the outer dark-matter halo and satellite plane, as is supported by Milky Way analogues from Auriga and TNG50. By allowing qDM(r) and pDM(r) to vary with radii, we find tentative evidence that the dark-matter halo is twisted. This agrees alignment with the disc in the inner regions and transitions to a vertical orientation at r > 20 kpc, supporting the disc flip scenario prediction. Such disc reorientation is non-trivial, yet its physical mechanism is straightforward to comprehend and naturally originates a vertical satellite plane. Our findings offer a unified framework that links dark-matter halo orientation, satellite alignment, and disc evolution, reinforcing the internal consistency of the Milky Way in the Λ cold dark matter model.
Key words: Galaxy: evolution / Galaxy: halo / Galaxy: kinematics and dynamics
© The Authors 2026
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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