ALMA CO observations of NGC 4565 reveal a thin non-flaring molecular disk with a central gap, consistent GMC properties to 17 kpc, and a prominent star-forming ring feature.
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Young star clusters in the NGC 628 simulation inherit a filament mass power-law index of -1.35 at formation via gravitational fragmentation and evolve to -1.55 after 60 Myr.
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The Radial and Vertical Structure of Molecular Gas in the Edge-On Galaxy NGC 4565
ALMA CO observations of NGC 4565 reveal a thin non-flaring molecular disk with a central gap, consistent GMC properties to 17 kpc, and a prominent star-forming ring feature.
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Revealing the Connection Between the Filamentary Hierarchy and Star Cluster Formation in a Simulated NGC 628 Galaxy
Young star clusters in the NGC 628 simulation inherit a filament mass power-law index of -1.35 at formation via gravitational fragmentation and evolve to -1.55 after 60 Myr.