We address the problem of the origin of massive stars, namely the origin, path, and
timescale of the mass flows that create them. Based on extensive numerical simulations, we …

Context. The star formation process leads to an increased chemical complexity in the
interstellar medium. Sites associated with high-mass star and cluster formation exhibit a so …

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 …

ALMA-IMF is an Atacama Large Millimeter/submillimeter Array (ALMA) Large Program
designed to measure the core mass function (CMF) of 15 protoclusters chosen to span their …

We present an overview of the CMZoom survey and its first data release. CMZoom is the first
blind, high-resolution survey of the Central Molecular Zone (CMZ; the inner 500 pc of the …

The stellar initial mass function (IMF) is critical to our understanding of star formation and the
effects of young stars on their environment. On large scales, it enables us to use tracers such …

Context. Classical hot cores are rich in molecular emission, and they show a high
abundance of complex organic molecules (COMs). The emergence of molecular complexity …

Aims. Thanks to the high angular resolution, sensitivity, image fidelity, and frequency
coverage of ALMA, we aim to improve our understanding of star formation. One of the …

We present the first data release of the ALMA-IMF Large Program, which covers the 12m-
array continuum calibration and imaging. The ALMA-IMF Large Program is a survey of …

Massive protostars attain high luminosities as they are actively accreting and the radiation
pressure exerted on the gas in the star's atmosphere may launch isotropic high-velocity …