Star clusters stand at the intersection of much of modern astrophysics: the ISM, gravitational
dynamics, stellar evolution, and cosmology. Here, we review observations and theoretical …

Star clusters are fundamental units of stellar feedback and unique tracers of their host
galactic properties. In this review, we will first focus on their constituents, ie detailed insight …

We use accurate estimates of aluminium abundance from the APOGEE Data Release 17
and Gaia Early Data Release 3 astrometry to select a highly pure sample of stars with …

As they grow, galaxies can transition from irregular/spheroidal with 'bursty'star formation
histories (SFHs), to discy with smooth SFHs. But even in simulations, the direct physical …

Abstract We introduce the MOdelling Star cluster population Assembly In Cosmological
Simulations within EAGLE (E-MOSAICS) project. E-MOSAICS incorporates models …

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 …

The standard cold dark matter plus cosmological constant model predicts that galaxies form
within dark-matter haloes, and that low-mass galaxies are more dark-matter dominated than …

We discuss some of the key open questions regarding the formation and evolution of
globular clusters (GCs) during galaxy formation and assembly within a cosmological …

We study the physical properties (size, stellar mass, luminosity, and star formation rate) and
scaling relations for a sample of 166 star-forming clumps with redshift z∼ 2–6.2. They are …

We present 25 cosmological zoom-in simulations of Milky-Way-mass galaxies in the
'MOdelling Star cluster population Assembly In Cosmological Simulations within EAGLE'(E …