<p>Extragalactic, unresolved GCs are possibly the simplest class of astrophysical objects beyond stars. As such, they are an important tool for understanding the formation and evolution of the host galaxies. Within the VST surveys FDS and VEGAS the study of such compact stellar systems, both for single bright galaxies (VEGAS) and for the 'entire' GC population in the Fornax cluster of galaxies (FDS), is in progress.<br> In my presentation, I will present and discuss the recent results for the characterization of GC properties (spatial distributions, colors, etc.) based on multiwavelength VST data from the two surveys, and describe the perspectives of future studies.</p
Abstract Context: A possible pathway for understanding the events and the mechanisms involved in ga...
The VEGAS-SSS programme is devoted to studying the properties of small stellar systems (SSSs) in and...
The superior resolution of HST and the light gathering power of large 8-10m class telescopes are now...
Extragalactic, unresolved GCs are possibly the simplest class of astrophysical objects beyond stars....
We present a study of globular clusters (GCs) and other small stellar systems (SSSs) in the field of...
We present a study of globular clusters (GCs) and other small stellar systems (SSSs) in the field of...
We present a study of globular clusters (GCs) and other small stellar systems (SSSs) in the field of...
We present a study of globular clusters (GCs) and other small stellar systems (SSSs) in the field of...
We present a study of globular clusters (GCs) and other small stellar systems (SSSs) in the field of...
We analyze the globular cluster (GC) systems in two very different galaxies, NGC 3115 and NGC 1399. ...
We analyze the globular cluster (GC) systems in two very different galaxies, N3115 and N1399. With ...
The Fornax Deep Survey (FDS) is a multi-band imaging survey of the Fornax cluster of galaxies, execu...
We analyze the globular cluster (GC) systems in two very different galaxies, NGC 3115 and NGC 1399. ...
In the era of deep photometric surveys aimed at studying galaxy structures down to the faintest leve...
Most of the globular clusters in the universe reside in gaint elliptical galaxies. The number of GCs...
Abstract Context: A possible pathway for understanding the events and the mechanisms involved in ga...
The VEGAS-SSS programme is devoted to studying the properties of small stellar systems (SSSs) in and...
The superior resolution of HST and the light gathering power of large 8-10m class telescopes are now...
Extragalactic, unresolved GCs are possibly the simplest class of astrophysical objects beyond stars....
We present a study of globular clusters (GCs) and other small stellar systems (SSSs) in the field of...
We present a study of globular clusters (GCs) and other small stellar systems (SSSs) in the field of...
We present a study of globular clusters (GCs) and other small stellar systems (SSSs) in the field of...
We present a study of globular clusters (GCs) and other small stellar systems (SSSs) in the field of...
We present a study of globular clusters (GCs) and other small stellar systems (SSSs) in the field of...
We analyze the globular cluster (GC) systems in two very different galaxies, NGC 3115 and NGC 1399. ...
We analyze the globular cluster (GC) systems in two very different galaxies, N3115 and N1399. With ...
The Fornax Deep Survey (FDS) is a multi-band imaging survey of the Fornax cluster of galaxies, execu...
We analyze the globular cluster (GC) systems in two very different galaxies, NGC 3115 and NGC 1399. ...
In the era of deep photometric surveys aimed at studying galaxy structures down to the faintest leve...
Most of the globular clusters in the universe reside in gaint elliptical galaxies. The number of GCs...
Abstract Context: A possible pathway for understanding the events and the mechanisms involved in ga...
The VEGAS-SSS programme is devoted to studying the properties of small stellar systems (SSSs) in and...
The superior resolution of HST and the light gathering power of large 8-10m class telescopes are now...