Dynamical Accretion Flows -- ALMAGAL: Flows along filamentary structures in high-mass star-forming clusters

We use data from the ALMA Evolutionary Study of High Mass Protocluster Formation in the Galaxy (ALMAGAL) survey to study 100 ALMAGAL regions at \sim 1 arsecond resolution located between \sim 2 and 6 kpc distance. Using ALMAGAL \sim 1.3mm line and continuum data we estimate flow rates onto individual... Show more