Supersonic turbulence and structure of interstellar molecular clouds

Details Supersonic turbulence and structure of interstellar molecular clouds Supersonic turbulence and structure of interstellar molecular clouds

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...200.7319p&link_type=abstract

American Astronomical Society, 200th AAS Meeting, #73.19; Bulletin of the American Astronomical Society, Vol. 34, p.769

Astronomy and Astrophysics

Astronomy

1

Scientific paper

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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