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Strikingly high fraction of fast rotators in Magellanic Cloud star clusters
Greta Ettorre, Alessandro Mazzi, Leo Girardi +14
There has been growing evidence that the rich star clusters in the Magellanic Clouds contain significant fractions of rapidly rotating stars. In this work, we aim to constrain thes…
Clusters, Clumps, Dust, & Gas (CCDG) in NGC1614: Bench-marking Cluster Demographics in Extreme Systems
Miranda Caputo, Rupali Chandar, Angus Mok +3
Observations of young star clusters in a variety of galaxies have been used to constrain basic properties related to star-formation, such as the fraction of stars found in clusters…
On the Precision of Full-Spectrum Fitting of Simple Stellar Populations. IV. A Systematic Comparison with Results from Colour-Magnitude Diagrams
Randa Asa'd, Paul Goudfrooij, A. M. As'ad
In this fourth paper of a series on the precision of ages of stellar populations obtained through the full-spectrum fitting technique, we present a first systematic analysis that c…
Role of host galaxy in the formation of multiple stellar populations: Analysis of NGC 1786 and NGC 1898
Viswajith Vanaraj, Florian Niederhofer, Paul Goudfrooij
Even after decades of research, the origin of multiple stellar populations in globular clusters remains enigmatic. The question as to whether the galaxy environment plays a role in…
On the Precision of Full-spectrum Fitting of Stellar Populations. III. Identifying Age Spreads
Randa Asa'd, Paul Goudfrooij, A. M. As'ad +4
In this third paper of a series on the precision of obtaining ages of stellar populations using the full spectrum fitting technique, we examine the precision of this technique in d…
The wide upper main sequence and main sequence turnoff of the ~ 800 Myr old star cluster NGC1831
Matteo Correnti, Paul Goudfrooij, Andrea Bellini +1
We present the analysis of the colour-magnitude diagram (CMD) morphology of the ~ 800 Myr old star cluster NGC1831 in the Large Magellanic Cloud, exploiting deep, high-resolution p…