Star and planet formation are inextricably linked. In the earliest phases of the collapse of a
protostar, a disc forms around the young star and such discs are observed for the first …

The Gaia mission has opened a new window into the internal kinematics of young star
clusters at the sub-km s− 1 level, with implications for our understanding of how star clusters …

We present a novel view on the morphology and dynamical state of ten prominent, nearby
(≤ 500 pc), and young (∼ 30–300 Myr) open star clusters with Gaia DR2: α Per, Blanco 1 …

Energetic feedback from star clusters plays a pivotal role in shaping the dynamical evolution
of giant molecular clouds (GMCs). To study the effects of stellar feedback on the star …

We present Ekster, a new method for simulating star clusters from birth in a live galaxy
simulation that combines the smoothed-particle hydrodynamics (SPH) method Phantom with …

In previous papers of this series, we developed a new algorithm for modelling the formation
of star clusters in galaxy formation simulations. Here we investigate how dissolution of …

We quantify the spatial distribution of stars for two subclusters centred around the
massive/intermediate-mass stars S Mon and IRS 1/2 in the NGC 2264 star-forming region …

The first stages of planet formation usually occur when the host star is still in a (relatively)
dense star-forming region, where the effects of the external environment may be important …

Many theoretical studies have shown that external photoevaporation from massive stars can
severely truncate, or destroy altogether, the gaseous protoplanetary disks around young …

Aims. We built Galactic open star cluster mass functions (CMFs) for different age sub-
samples and spatial locations in the wider solar neighbourhood. Here, we present a simple …