collaborators

11 papers

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.GA2026

Kinematic hints of a nuclear bar in the Milky Way

Karl Fiteni, Mattia C. Sormani, Victor P. Debattista +8

The Milky Way hosts a flattened nuclear stellar disc (NSD) that dominates the gravitational potential in the inner few hundred parsecs. Whether the NSD is purely axisymmetric or co…

astro-ph.GA2026

Kinematic diagnostics for non-axisymmetry in the Milky Way's nuclear stellar disc

Karl Fiteni, Xingchen Li, Mattia C. Sormani +8

There is now strong evidence that the Milky Way (MW) hosts a nuclear stellar disc (NSD). However, whether the NSD is purely axisymmetric or contains a nuclear bar remains unresolve…

astro-ph.GA2026

Geometry of the Milky Way's dark matter from dynamical models of the tilted stellar halo

Adam M. Dillamore, Jason L. Sanders

The shape and orientation of the Milky Way's dark matter halo remain poorly constrained. Observations of the accreted stellar halo show that it is triaxial and tilted with respect…

astro-ph.GA2025

Bar-driven dispersal of Galactic substructure

Adam M. Dillamore, Jason L. Sanders

Galactic archaeologists often assume that integrals of motion (IoMs) such as and are conserved, so substructure remains frozen in IoM space over many Gyr. However, this i…

astro-ph.GA2025

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon

Stephanie Monty, Allison L. Strom, Thomas M. Stanton +7

Our understanding of the chemical evolution of galaxies has advanced through measurements from both distant galaxies across redshift, and our own Milky Way (MW). To form a comprehe…