Dynamical Evolution of The Open Clusters Collinder 110 and NGC 2477

arXiv:2609.31925 · astro-ph.GA · Submitted 2026-09-25 · Read on arXiv

astro-ph.GA

Submitted: 2026-09-25

Updated: 2026-09-25

Code: https://github.com/msolpera/pyUPMASK

Terminology

• Mass Segregation — 28× in this paper · explained in 2 episodes
• Core — 22× in this paper · explained in 2 episodes
• Mass Function — 13× in this paper
• Metallicity — 8× in this paper · explained in 3 episodes
• Abundance — 4× in this paper · explained in 1 episode
• Calibration — 2× in this paper · explained in 7 episodes
• Radial Velocity Spectrometer — 2× in this paper
• Trace — 2× in this paper · explained in 2 episodes
• Benchmark — 1× in this paper · explained in 2 episodes
• Cluster expansion — 1× in this paper · explained in 2 episodes
• Clustering — 1× in this paper · explained in 2 episodes

Related papers

• Apparent Stability in Self-Gravitating Turbulence and the Evolution of Molecular Clouds
• Two sets of potential-density basis pairs for the study of radial perturbations in collisionless spherical stellar systems
• Constraining reionization-era Ly alpha escape with JELS-MUSE: a highly complete H alpha-selected sample at z about6.1
• Deriving volume density profiles of filaments from observed surface densities
• Little Red Dots and Supermassive Black Hole Seed Formation in Ultralight Dark Matter Halos
• MEGATRON: how the first stars can create an iron metallicity plateau in the smallest dwarf galaxies