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Cited article:

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PAH features within few hundred parsecs of active galactic nuclei

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Mean-field theory of turbulence from the variational principle and its application to the rotation of a thin fluid disk

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Effective viscosity from cloud-cloud collisions in 3D global smoothed particle hydrodynamics simulations

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SUSTAINING STAR FORMATION RATES IN SPIRAL GALAXIES: SUPERNOVA-DRIVEN TURBULENT ACCRETION DISK MODELS APPLIED TO THINGS GALAXIES

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EVOLUTION OF GASEOUS DISK VISCOSITY DRIVEN BY SUPERNOVA EXPLOSION. II. STRUCTURE AND EMISSIONS FROM STAR-FORMING GALAXIES AT HIGH REDSHIFT

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Radial Variation of Attenuation and Star Formation in the Largest Late‐Type Disks Observed with GALEX

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HiDensity Distribution Driven by Supernovae: A Simulation Study

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Magnetic Fields and Ionized Gas in the Inner Galaxy: An Outer Scale for Turbulence and the Possible Role of HiiRegions

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From the Circumnuclear Disk in the Galactic Center to thick, obscuring tori of AGNs

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