GMC clustering in galaxy disks is mostly set by large-scale galactic gas distribution, with stacked CO profiles showing an extended component beyond individual cloud sizes and stronger clustering around massive bound clouds.
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The Structure of Molecular Gas in PHANGS-ALMA Galaxies: Cloud Spacing, Two-Point Correlation and Stacked Intensity Profiles
GMC clustering in galaxy disks is mostly set by large-scale galactic gas distribution, with stacked CO profiles showing an extended component beyond individual cloud sizes and stronger clustering around massive bound clouds.