It remains unclear how galactic environment affects star formation and stellar cluster
properties. This is difficult to address in Milky Way-mass galaxy simulations because of …

Observations of clusters suffer from issues such as completeness, projection effects,
resolving individual stars, and extinction. As such, how accurate measurements and …

The earliest evolution of star clusters involves a phase of co-existence of both newly formed
stars, and the gas from which they are forming. Observations of the gas in such regions …

Recent studies have identified star clusters with multiple components based on accurate
spatial distributions and/or proper motions from Gaia Data Release 3 (DR3), utilizing diverse …

Understanding the formation and evolution of high-mass star clusters requires comparisons
between theoretical and observational data to be made. Unfortunately, while the full phase …