The sonic scale of interstellar turbulence

Understanding the physics of turbulence is crucial for many applications, including weather, industry and astrophysics. In the interstellar medium1,2, supersonic turbulence plays a crucial role in controlling the gas density and velocity structure, and ultimately the birth of stars3-8. Here we prese...

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Main Authors: Federrath, Christoph (Author) , Klessen, Ralf S. (Author) , Iapichino, Luigi (Author) , Beattie, James R. (Author)
Format: Article (Journal)
Language:English
Published: 11 January 2021
In: Nature astronomy
Year: 2021, Volume: 5, Issue: 4, Pages: 365-371
ISSN:2397-3366
DOI:10.1038/s41550-020-01282-z
Online Access:Resolving-System, lizenzpflichtig, Volltext: https://doi.org/10.1038/s41550-020-01282-z
Verlag, lizenzpflichtig, Volltext: https://www.nature.com/articles/s41550-020-01282-z
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Author Notes:Christoph Federrath, Ralf S. Klessen, Luigi Iapichino, James R. Beattie
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Summary:Understanding the physics of turbulence is crucial for many applications, including weather, industry and astrophysics. In the interstellar medium1,2, supersonic turbulence plays a crucial role in controlling the gas density and velocity structure, and ultimately the birth of stars3-8. Here we present a simulation of interstellar turbulence with a grid resolution of 10,0483 cells that allows us to determine the position and width of the sonic scale (â„“s)-the transition from supersonic to subsonic turbulence.
Item Description:Gesehen am 19.01.2021
Physical Description:Online Resource
ISSN:2397-3366
DOI:10.1038/s41550-020-01282-z