Nate Bastian

TL;DR: In this article, the authors present a spectroscopic study of the stellar cluster population of M82, the archetype starburst galaxy, based primarily on new Gemini-North multi-object spectroscopy of 49 star clusters.

TL;DR: In this paper, a subset of 15 simulations of galaxies and their star clusters from the E-MOSAICS project were examined, and it was shown that more massive accreted galaxies typically contribute younger and more metal rich GCs.

TL;DR: In this article, the authors fit the star formation history of the turn-off region and the red clump region independently, and found that in most cases, the age spreads inferred from red clumps are smaller than those that result from the turnoff region.

TL;DR: In this article, a study of the variation of spatial structure of stellar populations within dwarf galaxies as a function of the population age is presented, where the authors use deep Hubble Space Telescope/Advanced Camera for Surveys imaging of nearby dwarf galaxies in order to resolve individual stars and create composite colour-magnitude diagrams (CMDs) for each galaxy.

TL;DR: In this paper, the formation and early evolution of the most massive and dense young stellar clusters is studied, focusing on the role they can play in our understanding of star and planet formation as a whole.