NGC 796 is a massive young cluster located 59 kpc from us in the diffuse intergalactic
medium of the 1/5–1/10 Z☉ Magellanic Bridge, allowing us to probe variations in star …

We present structural parameters for the seven intermediate-age and old star clusters NGC
121, Lindsay 1, Kron 3, NGC 339, NGC 416, Lindsay 38, and NGC 419 in the Small …

Context. Analysis of ages and metallicities of star clusters in the Magellanic Clouds provide
information for studies on the chemical evolution of the Clouds and other dwarf irregular …

We present CCD photometry in the Washington C and T 1 filters for six star clusters (B 34,
NGC 256, NGC 265, NGC 294, IC 1611 and NGC 376) in the Small Magellanic Cloud (SMC) …

We present in this study flux-calibrated integrated spectra in the range (3600–6800) Å for 18
concentrated SMC clusters. Cluster reddening values were estimated by interpolation …

ABSTRACT The VISCACHA (VIsible Soar photometry of star Clusters in tApii and Coxi
HuguA) Survey is an ongoing project based on deep photometric observations of …

We investigate the precision of the ages and metallicities of 21 000 mock simple stellar
populations (SSPs) determined through full-spectrum fitting. The mock SSPs cover an age …

We investigate the degree of spatial correlation among extended structures in the Large
Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC). To this purpose, we work with …

Colour–magnitude diagrams in the Washington system are presented for the first time for
five star clusters projected on to the outer region of the Small Magellanic Cloud (SMC). The …

ABSTRACT The Magellanic Bridge is the nearest low-metallicity, tidally stripped
environment, offering a unique high-resolution view of physical conditions in merging and …