We review the current knowledge about nuclear star clusters (NSCs), the spectacularly
dense and massive assemblies of stars found at the centers of most galaxies. Recent …

Astronomy, being one of the oldest observational sciences, has collected a lot of data over
the ages. In recent times, it is experiencing a huge data surge due to advancements in …

We present the final sample of the Exploration of Local VolumE Satellites (ELVES) survey, a
survey of the dwarf satellites of a nearly volume-limited sample of Milky Way (MW)− like …

The structure of a dwarf galaxy is an important probe of the effects of stellar feedback and
environment. Using an unprecedented sample of 223 low-mass satellites from the ongoing …

We reliably extend the stellar mass–size relation over 0.2≤ z≤ 2 to low stellar mass
galaxies by combining the depth of Hubble Frontier Fields with the large volume covered by …

We use the IllustrisTNG cosmological hydrodynamical simulation to study the formation of
ultradiffuse galaxies (UDGs) in galaxy clusters. We supplement the simulations with a …

We study ultra-diffuse galaxies (UDGs) in zoom in cosmological simulations, seeking the
origin of UDGs in the field versus galaxy groups. We find that while field UDGs arise from …

We propose that the ultra-diffuse galaxy (UDG) population represents a set of satellite
galaxies born in∼ 1010− 1011 M⊙ haloes, similar to field dwarfs, which suffer a dramatic …

We present the properties of the globular clusters (GCs) and nuclear star clusters (NSCs) of
low-mass (10 5.5< M⋆< 10 8.5 M⊙) early-type satellites of Milky Way–like and small group …

Shadows in the Dark: Low-surface-brightness Galaxies Discovered in the Dark Energy Survey
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