PHANGS-Hα provides new narrow-band Hα imaging and derived star formation products for 65 nearby galaxies, validated against MUSE spectroscopy and serving as calibration reference for the PHANGS collaboration.
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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.
citing papers explorer
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The PHANGS-H{\alpha} survey. Ground-based narrow-band imaging of nearby star-forming galaxies
PHANGS-Hα provides new narrow-band Hα imaging and derived star formation products for 65 nearby galaxies, validated against MUSE spectroscopy and serving as calibration reference for the PHANGS collaboration.
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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.