Gas Accretion Can Drive Turbulence in Galaxies

Gas Accretion Can Drive Turbulence in Galaxies

The driving of turbulence in galaxies is deeply connected with the physics of feedback, star formation, outflows, accretion, and radial transport in disks. The velocity dispersion of gas in galaxies therefore offers a promising observational window into these processes. However, the relative importa...

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Bibliographic Details
Main Authors: John C. Forbes, Razieh Emami, Rachel S. Somerville, Shy Genel, Dylan Nelson, Annalisa Pillepich, Blakesley Burkhart, Greg L. Bryan, Mark R. Krumholz, Lars Hernquist, Stephanie Tonnesen, Paul Torrey, Viraj Pandya, Christopher C. Hayward
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Galaxy physics
Galaxy processes
Galaxy dynamics
Galaxy formation
High-redshift galaxies
Disk galaxies
Online Access:https://doi.org/10.3847/1538-4357/acb53e

Internet

https://doi.org/10.3847/1538-4357/acb53e

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