We analyzed a sample of 9418 fundamental-mode and first-overtone Classical Cepheids
from the OGLE-IV Collection of Classical Cepheids. The distance to each Cepheid was …

We present a catalog of Galactic star clusters, associations and candidates with 10978
entries. This multi-band catalog was constructed over 20 years, starting with visual …

The formation scenario of the Magellanic Bridge during an encounter between the Large
and Small Magellanic Clouds∼ 200 Myr ago, as proposed by N-body models, would be …

We present a catalog of star clusters, associations, and related extended objects in the
Small Magellanic Cloud (SMC) and the Magellanic Bridge with 2741 entries, a factor 2 more …

We report the discovery of a stellar overdensity 8° north of the centre of the Small Magellanic
Cloud (SMC; Small Magellanic Cloud Northern Over-Density; SMCNOD), using data from …

Galaxy interactions distort the distribution of baryonic matter and can affect star formation.
The nearby Magellanic Clouds are a prime example of an ongoing galaxy interaction …

We study the luminosity function of intermediate-age red clump stars using deep, near-
infrared photometric data covering∼ 20 deg2 located throughout the central part of the …

We present the results of a systematic Milky Way satellite search performed across an array
of publicly available wide-area photometric surveys. Our aim is to complement previous …

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 …

Globular clusters (GCs) are proxies of the formation assemblies of their host galaxies.
However, few studies exist targeting GC systems of spiral galaxies up to several effective …