We use 3D hydrodynamical models to investigate the effects of massive star feedback from
winds and supernovae on inhomogeneous molecular material left over from the formation of …

We examine the evidence offered for triggered star formation against the backdrop provided
by recent numerical simulations of feedback from massive stars at or below giant molecular …

ABSTRACT The Milky Way Project citizen science initiative recently increased the number of
known infrared bubbles in the inner Galactic plane by an order of magnitude compared to …

Context. Feedback from massive stars affects the interstellar medium (ISM) from the
immediate surroundings of the stars (parsec scales) to galactic (kiloparsec) scales. High …

We identify hierarchical structures in the Vela OB2 complex and the cluster pair Collinder
135 and UBC 7 with Gaia EDR3 using the neural network machine-learning algorithm …

Cosmic rays (CR) are energetic nuclei that permeate the entire Galactic disk. Their existence
requires the presence of powerful particle accelerators. While Galactic supernova …

We present a detailed study of star formation occurring in bound star-forming clouds under
the influence of internal ionizing feedback from massive stars across a spectrum of cloud …

Aims. As part of the Herschel guaranteed time key programme “HOBYS”, we present the
PACS and SPIRE photometric survey of the star-forming region Vela-C, one of the nearest …

We present near-infrared multi-object spectroscopy and JHK s imaging of the massive stellar
content of the Galactic star-forming region W3 Main, obtained with LUCI at the Large …

Aims. Massive stars form in clusters, and they are often found in different evolutionary stages
located close to each other. To understand evolutionary and environmental effects during …