Abstract
The interstellar medium provides a unique laboratory for highly supersonic, driven hydrodynamic turbulence. We propose a theory of such turbulence, test it by numerical simulations, and use the results to explain observational scaling properties of interstellar molecular clouds, the regions where stars are born.
Keywords
Supersonic speedPhysicsMolecular cloudTurbulenceInterstellar mediumInterstellar cloudStarsAstrophysicsScalingAstronomyComputational physicsMechanicsGalaxy
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Publication Info
- Year
- 2002
- Type
- article
- Volume
- 89
- Issue
- 3
- Pages
- 031102-031102
- Citations
- 85
- Access
- Closed
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Cite This
Stanislav Boldyrev,
Åke Nordlund,
Paolo Padoan
(2002).
Supersonic Turbulence and Structure of Interstellar Molecular Clouds.
Physical Review Letters
, 89
(3)
, 031102-031102.
https://doi.org/10.1103/physrevlett.89.031102
Identifiers
- DOI
- 10.1103/physrevlett.89.031102