Unbound young stellar systems, the loose ensembles of physically related young bright
stars, trace the typical regions of recent star formation in galaxies. Their morphologies vary …

The microphysics of∼ GeV cosmic ray (CR) transport on galactic scales remain deeply
uncertain, with almost all studies adopting simple prescriptions (eg constant diffusivity). We …

We present a study correlating the spatial locations of young star clusters with those of
molecular clouds in NGC 5194, in order to investigate the time-scale over which clusters …

We present an analysis of the global and spatially resolved Kennicutt–Schmidt (KS) star
formation relation in the FIRE (Feedback In Realistic Environments) suite of cosmological …

We present three-dimensional radiation-hydrodynamical simulations of the impact of stellar
winds, photoelectric heating, photodissociating and photoionizing radiation, and …

We present observational evidence of a correlation between the high-mass slope of the
stellar initial mass function (IMF) in young star clusters and their stellar surface density, σ …

We present radiation-magneto-hydrodynamic simulations of star formation in self-gravitating,
turbulent molecular clouds, modelling the formation of individual massive stars, including …

Context. Massive stars are among the main cosmic engines driving the evolution of star-
forming galaxies. Their powerful ionising radiation and stellar winds inject a large amount of …

We investigate the origin of observed local star formation relations using radiative
magnetohydrodynamic simulations with self-consistent star formation and ionizing radiation …

We present optical photometry and spectroscopy of SN 2016iet (= Gaia16bvd= PS17brq), an
unprecedented Type I supernova (SN I) at z= 0.0676 with no obvious analog in the existing …