We use 3D radiation hydrodynamic (RHD) simulations to study the formation of massive star
clusters under the combined effects of direct ultraviolet (UV) and dust-reprocessed infrared …

We analyze image and spectral data from≈ 365 ks of observations from the Chandra X-ray
Observatory of the nearby, edge-on starburst galaxy NGC 253 to constrain properties of the …

The center of the nearby galaxy NGC 253 hosts a population of more than a dozen super
star clusters (SSCs) that are still in the process of forming. The majority of the star formation …

Context. Phosphorus (P) is a crucial element for life given its central role in several
biomolecules. P-bearing molecules have been discovered in different regions of the Milky …

We present a spatially resolved excitation analysis for the central molecular zone (CMZ) of
the starburst galaxy NGC 253 using the data from the Atacama Large Millimeter …

Context. Sulphur-bearing species are detected in various environments within Galactic star-
forming regions and are particularly abundant in the gas phase of outflow and shocked …

Henize 2–10 is a dwarf starburst galaxy hosting a∼ 10 6 M⊙ black hole (BH) that is driving
an ionized outflow and triggering star formation within the central∼ 100 pc of the galaxy …

We present a set of controlled hydrodynamical simulations to study the effects of strong
galactic outflows on the density and temperature structures, and associated X-ray …

The star formation rate (SFR) is a fundamental parameter for describing galaxies and
inferring their evolutionary course. H ii regions yield the best measure of instantaneous SFR …

Self-enrichment is one of the leading explanations for chemical anomalies in globular
clusters. In this scenario, various candidate polluter stars have been proposed to eject gas …