Investigating the Young Stellar Populations and Hierarchies in Nearby Galaxies with the UVIT. III. Evidence for a Largest Scale of Correlated Stellar Structures and a Non-universal Fractal Dimension

arXiv:2609.01065 · astro-ph.GA · Submitted 2026-09-01 · Read on arXiv

astro-ph.GA

Submitted: 2026-09-01

Updated: 2026-09-01

Terminology

Stellar Feedback — 8× in this paper · explained in 2 episodes
Clustering — 6× in this paper · explained in 2 episodes
Robustness — 4× in this paper · explained in 5 episodes
Dust Attenuation — 2× in this paper · explained in 2 episodes
Metallicity — 2× in this paper · explained in 3 episodes
Trace — 2× in this paper · explained in 2 episodes
Accuracy — 1× in this paper · explained in 1 episode
Aperture — 1× in this paper · explained in 1 episode
Aperture Photometry — 1× in this paper · explained in 1 episode
LMC and Small Magellanic Cloud — 1× in this paper
Large Magellanic Cloud — 1× in this paper
Velocity Dispersion — 1× in this paper · explained in 2 episodes

Sources

Related papers