Globular clusters (GCs) exhibit star-to-star variations in specific elements (eg, He, C, N, O,
Na, Al) that bear the hallmark of high-temperature H-burning. These abundance variations …

Young massive clusters (YMCs) are dense aggregates of young stars that form the
fundamental building blocks of galaxies. Several examples exist in the Milky Way Galaxy …

We update the capabilities of the open-knowledge software instrument Modules for
Experiments in Stellar Astrophysics (MESA). The new auto _ diff module implements …

To reach a deeper understanding of the origin of elements in the periodic table, we construct
Galactic chemical evolution (GCE) models for all stable elements from C (A= 12) to U (A …

The chemical evolution of the Universe is governed by the chemical yields from stars, which
in turn are determined primarily by the initial stellar mass. Even stars as low as 0.9 M⊙ can …

Context. The post-asymptotic giant branch (AGB) phase is arguably one of the least
understood phases of the evolution of low-and intermediate-mass stars. The two grids of …

We present a model for the concurrent formation of globular clusters (GCs) and
supermassive stars (SMSs,≳ 103 M⊙) to address the origin of the HeCNONaMgAl …

An updated grid of stellar yields for low-to intermediate-mass thermally pulsing asymptotic
giant branch (AGB) stars is presented. The models cover a range in metallicity Z= 0.02 …

During the commissioning of JWST, the medium-resolution spectrometer (MRS) on the mid-
infrared instrument (MIRI) observed the planetary nebula SMP LMC 058 in the Large …

We study the dust content of galaxies from z= 0 to z= 9 in semi-analytic models of galaxy
formation that include new recipes to track the production and destruction of dust. We …