Recent work on metal-intermediate globular clusters (GCs) with [Fe/H]=− 1.5 and− 0.75 has
illustrated the theoretical behavior of multiple populations in photometric diagrams obtained …

Abstract We present the Sloan Digital Sky Survey V Local Volume Mapper (LVM). The LVM
is an integral-field spectroscopic survey of the Milky Way, Magellanic Clouds, and a sample …

Abstract James Webb Space Telescope (JWST) observations have been demonstrated to
be efficient in detecting multiple stellar populations in globular clusters (GCs) in the low …

Young and intermediate-age star clusters of both Magellanic Clouds exhibit complex colour–
magnitude diagrams. In addition to the extended main-sequence turn-offs (eMSTOs) …

The chemical evolution history of the Small Magellanic Cloud (SMC) has been a matter of
debate for decades. The challenges in understanding the SMC chemical evolution are …

About one-fifth of the Galactic globular clusters (GCs), dubbed Type II GCs, host distinct
stellar populations with different heavy elements abundances. NGC 1851 is one of the most …

Binary stars play a major role in determining the dynamic evolution of star clusters. We used
images collected with the Hubble Space Telescope to study fourteen star clusters of the …

The origin of extended main-sequence turn-offs (eMSTO) in star clusters younger than 2 Gyr
still challenges our current understanding of stellar evolution. Exploiting data from Gaia Data …

Context. The Magellanic Clouds (MCs) are the Milky Way's most massive dwarf satellites. As
they also represent the closest pair of galaxies in an ongoing tidal interaction while …

The detection of split main sequences (MSs) associated with young clusters (≲ 600 Myr) has
attracted a lot of attention. A prevailing scenario is that a bimodality of stellar rotation …