Parameters of the Supernova-Driven Interstellar Turbulence
Galactic dynamo models take as input certain parameters of the interstellar turbulence, most essentially the correlation time <inline-formula><math display="inline"><semantics><mi>τ</mi></semantics></math></inline-formula>, root-mean-square t...
Main Authors: | Luke Chamandy, Anvar Shukurov |
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Format: | Article |
Language: | English |
Published: |
MDPI AG
2020-07-01
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Series: | Galaxies |
Subjects: | |
Online Access: | https://www.mdpi.com/2075-4434/8/3/56 |
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