Computer Science
Scientific paper
Dec 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jfm...245....1b&link_type=abstract
Journal of Fluid Mechanics (ISSN 0022-1120), vol. 245, p. 1-28.
Computer Science
39
Gravitational Collapse, Interstellar Gas, Isotropic Turbulence, Molecular Clouds, Gravitational Constant, Jeans Theory, Kinetic Energy, Turbulent Flow
Scientific paper
The conditions for gravitational instability in a statistically homogeneous turbulent fluid is investigated using a renormalization technique, with particular reference to the problem of stability of molecular clouds and the origin of protostellar density fluctuations. It is shown how turbulence at scales smaller than the potentially collapsing scale builds up a turbulent pressure force that effectively resists compression if the kinetic energy is sufficient to balance gravitational attraction.
Bonazzola Silvano
Falgarone Edith
Heyvaerts Jean
Panis Jean-François
Pérault Michel
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