Context. HCN, HNC, and their isotopologues are ubiquitous molecules that can serve as
chemical thermometers and evolutionary tracers to characterize star-forming regions …

Context. High-mass star formation is far less understood than low-mass star formation. It
entails the ejection of matter through molecular outflows, which disturbs the protostellar …

Context. Star-forming molecular clouds are characterised by the ubiquity of intertwined
filaments. The filaments have been observed in both high-and low-mass star-forming …

Context. Electron fraction and cosmic-ray ionization rates in star-forming regions are
important quantities in astrochemical modeling and are critical to the degree of coupling …

Interstellar shocks, a key element of stellar feedback processes, shape the structure of the
interstellar medium (ISM) and are essential for the chemistry, thermodynamics, and …

We present the outflows detected in HOPS 373SW, a protostar undergoing a modest 30%
brightness increase at 850 μm. Atacama Large Millimeter/submillimeter Array observations …

Context. The SiO emissions are usually used to trace high-velocity outflow shocks in star-
forming regions. However, several studies have found low-velocity and widespread SiO …

The production of silicon monoxide (SiO) can be considered as a fingerprint of shock
interaction. In this work, we use high-sensitivity observations of the SiO (2–1) and H CO (1 …

The exploration of outflows in protobinary systems presents a challenging yet crucial
endeavour, offering valuable insights into the dynamic interplay between protostars and …

Context. Understanding the connection between outflows, winds, accretion, and discs in the
inner protostellar regions is crucial for comprehending star and planet formation processes …