Galaxies are embedded within halos of dark matter, and the tilt of those halos can affect the galaxy’s stellar halo and stellar disk.
Galaxies are embedded within halos of dark matter, the invisible matter thought to make up 85% of the mass of our universe. New research investigates how a tilt in a galaxy’s dark matter halo can affect its stellar halo and stellar disk.
Nestled in a Halo of Dark Matter
Spiral galaxies like the Milky Way have a beautifully nested structure. A thin and extended disk of stars is enveloped within a thicker disk of older stars that is then wrapped up within an expansive galactic halo. Underlying all of this structure is the part of the galaxy that we can’t see: the dark matter halo in which our galaxy is embedded.
While the goings-on in our galaxy’s dark matter halo might seem far removed from life in the thin stellar disk, research by Jiwon Jesse Han (Center for Astrophysics, Harvard & Smithsonian) and collaborators has explored the connection between the two. In a recent article, Han’s team examined the alignment between galaxies’ stellar disks and the inner regions of their dark matter halos and probed what it might mean if the two are misaligned.
Tilting Halos with Ancient Mergers
Using the TNG50 cosmological simulation — part of the IllustrisTNG suite of cosmological simulations — Han’s team selected synthetic galaxies that are similar to the Milky Way and our neighboring galaxy, Andromeda. The simulated galaxies have masses similar to the Milky Way’s present-day mass, a disk-like appearance, and don’t have any other massive galaxies within 500 kiloparsecs (1.6 million light-years).
For each of these Milky Way siblings, 198 in all, the team measured the angle between the inner dark halo (the part of the halo within 50 kiloparsecs or 160,000 light-years of the stellar disk), the stellar halo, and the stellar disk. Over 6 billion years of simulation time, the tilt angles between the galaxies’ inner dark halos and their stellar disks, and between their stellar halos and their stellar disks, varied. But the inner dark halos and the stellar halos showed similar behavior, tilting and whirling in tandem.
The Milky Way’s stellar halo is currently tilted relative to its stellar disk at an angle of about 20–30 degrees. Given the parallel behavior of dark halos and stellar halos, this implies that the Milky Way’s inner dark halo is tilted relative to its stellar disk at about 20 degrees. What effect does a tilted dark halo have?
Warped Disks and the Milky Way
Han and collaborators delved deeper into the simulation, focusing on the behavior of a single Milky Way analog that experienced a merger 7 billion years ago. The merger tilted the galaxy’s dark matter halo by 50 degrees, and the stellar halo followed suit, swayed by the gravitational pull of the dark halo. Over time, and under the influence of friction, torque, and other factors, the tilts of the dark and stellar halos shrank to 20 degrees.
The effects of the tilted dark matter halo were felt in the thin stellar disk, as well: a few billion years post merger, a warp appeared in the previously flat disk. This warp lessened slightly over time but persisted until the present day in the simulation.
Like the simulated galaxy studied here, the Milky Way experienced a merger billions of years ago and today sports a warped disk. Based on the results of the simulation, Han’s team proposed that halo-tilting mergers induce the long-lasting warps in galactic disks seen in more than half of all spiral galaxies today.
“Tilted Dark Halos Are Common and Long-Lived, and Can Warp Galactic Disks,” Jiwon Jesse Han et al 2023 ApJL 957 L24. doi:10.3847/2041-8213/ad0641