The star formation histories of fossil group galaxies
A comparison is carried out among the star formation histories of early-type galaxies in fossil groups, clusters and low density environments. Although they...
The star formation histories of quiescent ultra-diffuse galaxies and their dependence on environment and globular cluster richness
We derive the stellar population parameters of 11 quiescent ultra-diffuse galaxies (UDGs) from Keck/KCWI data. We supplement these with 14 literature UDGs...
The star formation history and dust content in the far outer disc of M31
We present a detailed analysis of two fields located 26 kpc (˜5 radial scalelengths) from the centre of M31 along the south-west semimajor axis of the disc. One...
The Star Formation History and Dust Production in Andromeda IX
Local Group (LG), the nearest and most complete galactic environment, provides valuable information on the formation and evolution of the Universe. Studying...
The star formation history and evolution of the circumnuclear region of M100
Context. Star-forming nuclear rings in barred galaxies are common in nearby spirals, and their detailed study can lead to important insights into the evolution...
The Star Formation History and Morphological Evolution of the Draco Dwarf Spheroidal Galaxy
The photometric and morphological properties, as well as the star formation history, of the Draco dwarf spheroidal galaxy are analyzed on the basis of wide...
The Star Formation History and Spatial Distribution of Stellar Populations in the Ursa Minor Dwarf Spheroidal Galaxy
As a part of a project devoted to the study of the Ursa Minor dwarf spheroidal (dSph) galaxy, the star formation history of the galaxy is presented. The...
The star formation history from resolved stellar populations. State of the art and future perspectives
We present a new method to solve the star formation history (SFH) of a complex stellar population system from the analysis of the color-magnitude diagram (CMD)...
We present a quantitative analysis of the star formation history (SFH) of 12 fields in the Small Magellanic Cloud (SMC) based on unprecedented deep [(B-R),R]...