Introducing AuriGLOBES: The effects of compressive tides, compact object-induced mass loss, and size evolution on modelling globular clusters

arXiv:2606.30746 · astro-ph.GA, physics.comp-ph · Submitted 2026-06-29 · Read on arXiv

astro-ph.GA, physics.comp-ph

Submitted: 2026-06-29

Updated: 2026-07-27

Comments: 23 pages, 22 figures. Accepted for publication in A&A

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

Metallicity — 27× in this paper · explained in 3 episodes
Milky Way — 9× in this paper
Velocity Dispersion — 4× in this paper · explained in 2 episodes
Stellar Feedback — 2× in this paper · explained in 2 episodes
Trace — 2× in this paper · explained in 2 episodes
Accuracy — 1× in this paper · explained in 1 episode
Alignment — 1× in this paper · explained in 1 episode
Canadian Institute for Theoretical Astrophysics — 1× in this paper
Degeneracy — 1× in this paper · explained in 3 episodes
Distribution Shift — 1× in this paper · explained in 5 episodes
Gaussian Mixture Model (GMM) — 1× in this paper · explained in 2 episodes
Modularity — 1× in this paper · explained in 9 episodes
N-body simulations — 1× in this paper · explained in 2 episodes
Star Formation Rate (SFR) — 1× in this paper · explained in 5 episodes
Young Star Clusters — 1× in this paper

Sources

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