3D Mapping of the Dynamic Feedback and Chemistry in the Star Formation Process across Galaxy Disks

The PHANGS-MUSE observational programme, is a survey using the MUSE integral field spectrograph at the VLT to map 19 star-forming disk galaxies (Emsellem et al. 2021, arXiv:2110.03708). Together with dedicated ALMA and HST observations delivering exquisite information regarding, e.g., giant molecular clouds and star clusters, the MUSE campaign provides a comprehensive view of the chemo-dynamical evolution of the star formation process across the different environments, addressing timescales associated with star formation, quantifying the importance of stellar feedback, studying the chemical enrichment and mixing, and connecting the local conditions with the large-scale dynamics. Please find additional information, including on data types, in the data Release Description (https://www.eso.org/rm/api/v1/public/releaseDescriptions/184) and in Emsellem et al. 2022 (A&A, 659, 191; https://ui.adsabs.harvard.edu/abs/2022A%26A...659A.191E/abstract).