Galactic winds from star-forming galaxies are crucial to the process of galaxy formation and
evolution, regulating star formation, shaping the stellar mass function and the mass …

The Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) is a blind narrow-
band (NB) Hα+[NII] imaging survey carried out with MegaCam at the Canada–France …

We describe new Hi-GAL based maps of the entire Galactic Plane, obtained using
continuum data in the wavelength range 70–500 μm. These maps are derived with the …

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 …

Stellar feedback is needed to produce realistic giant molecular clouds and galaxies in
simulations, but due to limited numerical resolution, feedback must be implemented using …

Context. Star formation and stellar feedback are interlinked processes that redistribute
energy, turbulence, and material throughout galaxies. Because young and massive stars …

We study the IB (s) m galaxy IC 3476 observed in the context of the Virgo Environmental
Survey Tracing Ionised Gas Emission (VESTIGE), a blind narrow-band Hα+[NII] imaging …

Context. The nature of turbulence in molecular clouds is one of the key parameters that
control star formation efficiency: compressive motions, as opposed to solenoidal motions …

The morphology of H ii regions around young star clusters provides insight into the time-
scales and physical processes that clear a cluster's natal gas. We study∼ 700 young …

Molecular cloud structure is regulated by stellar feedback in various forms. Two of the most
important feedback processes are UV photoionization and supernovae from massive stars …