We review the current knowledge about nuclear star clusters (NSCs), the spectacularly
dense and massive assemblies of stars found at the centers of most galaxies. Recent …

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 …

We describe a public data release of the FIRE-2 cosmological zoom-in simulations of galaxy
formation (available at http://flathub. flatironinstitute. org/fire) from the Feedback In Realistic …

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 …

Increasingly, uncertainties in predictions from galaxy formation simulations (at sub-Milky
Way masses) are dominated by uncertainties in stellar evolution inputs. In this paper, we …

We present the escape fraction of hydrogen ionizing photons (f esc) from a sample of 34
high-resolution cosmological zoom-in simulations of galaxies at z≥ 5 in the Feedback in …

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 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 a large suite of magnetohydrodynamic simulations of turbulent, star-forming
giant molecular clouds (GMCs) with stellar feedback, extending previous work by simulating …