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P. Padoan (JPL, Caltech), S. Boldyrev (ITP, UCSB), A. Nordlund (Copenhagen Astronomical Observatory and Theoretical Astrophysics Center)
The interstellar medium provides unique laboratory for highly supersonic, driven hydrodynamics turbulence. We present a theory of such turbulence, confirm it by numerical simulations, and use the results to explain observational properties of interstellar molecular clouds, the regions where stars are born.
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Bulletin of the American Astronomical Society, 34
© 2002. The American Astronomical Soceity.