Nate Bastian

TL;DR: In this article, the authors introduce the MOdelling Star cluster population Assembly In Cosmological Simulations within EAGLE (E-MOSAICS) project, which incorporates models describing the formation, evolution, and disruption of star clusters into the eagle galaxy formation simulations, enabling the examination of the co-evolution of star cluster and their host galaxies in a fully cosmological context.

TL;DR: Alfred P. Sloan Foundation, National Science Foundation, US Department of Energy Office of Science, University of Arizona, Brazilian Participation Group, Brookhaven National Laboratory; University of Cambridge; Carnegie Mellon University; University Of Florida; French Participation Group; German Participation Group and Harvard University; Instituto de Astrofisica de Canarias; Michigan State/Notre Dame/JINA Participation Group as discussed by the authors.

TL;DR: In this paper, the authors analyse hydrodynamical simulations of turbulent fragmentation in star-forming regions to assess the dynamical properties of the resulting population of stars and (sub)clusters.

TL;DR: In this paper, it was shown that stellar rotation in stars with masses between 1.2-1.7 Msun can mimic the effect of a double or multiple population, whereas in actuality only a single population exists.

TL;DR: In this article, the authors make use of existing multi-wavelength data including recently available far-IR continuum and mm spectral line (H2O Southern Galactic Plane Survey and Millimetre Astronomy Legacy Team 90 GHz Survey) data and present new, deep, multiple-filter, near-IR (Very Large Telescope/NACO) observations to study G0.253 + 0.016.