Planet-forming disc evolution is not independent of the star formation and feedback process
in giant molecular clouds. In particular, OB stars emit UV radiation that heats and disperses …

Giant molecular clouds (GMCs) are the sites of star formation and stellar feedback in
galaxies. Their properties set the initial conditions for star formation and their lifecycles …

It is a major open question which physical processes stop gas accretion on to giant
molecular clouds (GMCs) and limit the efficiency at which gas is converted into stars. While …

The feedback from young stars (ie pre-supernova) is thought to play a crucial role in
molecular cloud destruction. In this paper, we assess the feedback mechanisms acting …

Modelling galaxy formation in hydrodynamic simulations has increasingly adopted various
radiative transfer methods to account for photoionization feedback from young massive …

Hydrogen emission lines can provide extensive information about star-forming galaxies in
both the local and high-redshift Universe. We present a detailed Lyman continuum (LyC) …

Our Sun lies within 300 parsecs of the 2.7-kiloparsecs-long sinusoidal chain of dense gas
clouds known as the Radcliffe Wave. The structure's wave-like shape was discovered using …

We present a high-resolution view of bubbles within the Phantom Galaxy (NGC 628), a
nearby (∼ 10 Mpc), star-forming (∼ 2 M⊙ yr− 1), face-on (i∼ 9) grand-design spiral galaxy …

We present a novel method for including the effects of early (pre-supernova) feedback in
simulations of galaxy evolution. Rather than building a model which attempts to match …

Context. The star cluster initial mass function is observed to have an inverse power law
exponent around 2, yet there is no consensus on what determines this distribution, and why …