Star clusters are fundamental units of stellar feedback and unique tracers of their host
galactic properties. In this review, we will first focus on their constituents, ie detailed insight …

Unbound young stellar systems, the loose ensembles of physically related young bright
stars, trace the typical regions of recent star formation in galaxies. Their morphologies vary …

The first JWST observations of nearby galaxies have unveiled a rich population of bubbles
that trace the stellar-feedback mechanisms responsible for their creation. Studying these …

We introduce the LYRA project, a new high-resolution galaxy formation model built within
the framework of the cosmological hydrodynamical moving mesh code arepo. The model …

We present a study correlating the spatial locations of young star clusters with those of
molecular clouds in NGC 5194, in order to investigate the time-scale over which clusters …

The analysis of star cluster ages in tandem with the morphology of their H ii regions can
provide insight into the processes that clear a cluster's natal gas, as well as the accuracy of …

We present an investigation of the relationship between giant molecular cloud (GMC)
properties and the associated stellar clusters in the nearby flocculent galaxy NGC 7793. We …

ABSTRACT A long-standing problem when deriving the physical properties of stellar
populations is the degeneracy between age, reddening, and metallicity. When a single …

Abstract We combine archival Hubble Space Telescope and new James Webb Space
Telescope imaging data covering the ultraviolet to mid-infrared regime to morphologically …

The sensitivity and angular resolution of photometric surveys executed by the Hubble Space
Telescope (HST) enable studies of individual star clusters in galaxies out to a few tens of …