activity
20242026
collaborators

9 papers

astro-ph.GA2026

SchwarMAX: a GPU-friendly Schwarzschild orbit-superposition modelling framework

HanYuan Zhang, David Chemaly, Eugene Vasiliev +3

The Schwarzschild orbit-superposition method is a highly flexible dynamical modelling tool. It constrains the mass distribution of a galaxy using line-of-sight velocity and photome…

astro-ph.GA2026

Enhanced rates of stellar radial migration in gas-rich discs at high redshift

HanYuan Zhang, Thor Tepper-García, Vasily Belokurov +6

Radial migration and dynamical heating redistribute stars within galactic discs and thereby modify the chemo-kinematic structure of their host galaxies. Usually, these secular proc…

astro-ph.GA2025

Orbital migration and heating history of the Galactic disc: a transition between the bimodal discs

HanYuan Zhang, Vasily Belokurov, Jason L. Sanders +7

Stellar orbits in the Galactic disc evolve from their birth to the current shape through both radial migration and dynamical heating. The history of their secular evolution is impr…

astro-ph.SR2025

Revealing the ages of metal-rich RR Lyrae via kinematic label transfer

HanYuan Zhang, Giuliano Iorio, Vasily Belokurov +3

RR Lyrae stars have long been considered reliable tracers of old, metal-poor populations, primarily due to their prevalence in globular clusters and the Galactic halo. However, the…

astro-ph.GA2025

Blind source separation of the stellar halo

Elliot Y. Davies, Vasily Belokurov, Andrey Kravtsov +4

The stellar halo of the Milky Way comprises an abundance of chemical signatures from accretion events and \textit{in-situ} evolution, that form an interweaving tapestry in kinemati…

astro-ph.GA2025

Observational Constraints of Radial Migration in the Galactic Disc Driven by the Slowing Bar

HanYuan Zhang, Vasily Belokurov, N. Wyn Evans +7

Radial migration is an important dynamical effect that has reshaped the Galactic disc, but its origin has yet to be elucidated. In this work, we present evidence that resonant drag…