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Context. Protoplanetary disks in dense, massive star-forming regions are strongly affected by their environment. How this environmental impact changes over time is an important constraint on disk evolution and external photoevaporation models. Aims. We characterize the dust emission from 179 disks in the core of the young (0.5 Myr) NGC 2024 cluster. By studying how the disk mass varies within the cluster, and comparing these disks to those in other regions, we aim to determine how external photoevaporation influences disk properties over time. Methods. Using the Atacama Large Millimeter/submillimeter Array, a 2.9′× 2.9′ mosaic centered on NGC 2024 FIR 3more »
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Wang, J. J. ; Vigan, A. ; Lacour, S. ; Nowak, M. ; Stolker, T. ; De Rosa, R. J. ; Ginzburg, S. ; Gao, P. ; Abuter, R. ; Amorim, A. ; et al ( , The Astronomical Journal)