Feedback from high-mass star-forming regions
The ALMA large program ALMAGAL has surveyed more then 1000 candidate high-mass star-forming regions in our Galaxy, based on properties revealed by the Herschel survey of the Milky Way, Hi-GAL. This large data set allows to derive statistically robust properties of a representative sample. I will present first results on the impact of radiative and mechanical feedback by discussing statistics on temperature distributions, the correlation with HII regions and outflow properties.
