How stars formed in warps settle into (and contaminate) thick discs
Tigran Khachaturyants, Leandro Beraldo e Silva, Victor P., Debattista

TL;DR
This study uses simulations to show how stars formed in the Milky Way's warp settle into the disc, contaminate the thick disc, and migrate radially, affecting the galaxy's stellar distribution and age gradients.
Contribution
It provides a detailed dynamical model of warp star settling, phase mixing, and radial migration, revealing their impact on the thick disc and stellar populations.
Findings
Warp stars tilt and align with the disc within ~1 Gyr.
They phase mix into an axisymmetric distribution over ~6 Gyr.
Warp stars are present throughout the disc, including the Solar Neighbourhood.
Abstract
In recent years star formation has been discovered in the Milky Way's warp. These stars formed in the warp (warp stars) must eventually settle into the plane of the disc. We use an -bodysmooth particle hydrodynamics model of a warped galaxy to study how warp stars settle into the disc. By following warp stars in angular momentum space, we show that they first tilt to partially align with the main disc in a time scale of Gyr. Then, once differential precession halts this process, they phase mix into an axisymmetric distribution on a time scale of Gyr. The warp stars end up contaminating the geometric thick disc. Because the warp in our fiducial simulation is growing, the {\it warp stars} settle to a distribution with a negative vertical age gradient as younger stars settle further from the mid-plane. While vertically extended, warp star orbits are still nearly…
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