Analyzing resolved stellar populations across the disk of a galaxy can provide unique
insights into how that galaxy assembled its stellar mass over its lifetime. Previous work at∼ …

We present a far-ultraviolet (FUV) study of 16 star-forming dwarf galaxies (SFDGs) using the
Ultra Violet Imaging Telescope. Morphologically, SFDGs are classified as dwarf spirals …

We explore the growth of the stellar disks in 14 nearby spiral galaxies as part of the
Deciphering the Interplay between the Interstellar medium, Stars, and the Circumgalactic …

This multiwavelength study of the star formation and star formation history (SFH) trends in
the nearby universe looks at nine nearby late-type spirals. Spectral energy distributions fitted …

Stellar feedback is fundamental to the modeling of galaxy evolution as it drives turbulence
and outflows in galaxies. Understanding the timescales involved are critical for constraining …