Hydrodynamical Simulations of Molecular Dynamics in Supersonic Turbulent Flow

Details Hydrodynamical Simulations of Molecular Dynamics in Supersonic Turbulent Flow Hydrodynamical Simulations of Molecular Dynamics in Supersonic Turbulent Flow

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.292...69p&link_type=abstract

Astrophysics and Space Science, v. 292, Issue 1, p. 69-75 (2004).

Astronomy and Astrophysics

Astrophysics

1

Hydrodynamics, Turbulence, Molecular Processes, Clouds, Ism

Scientific paper

Here we present results from simulations of turbulence in starforming environments obtained by coupling three-dimensional hydrodynamical models with appropriate chemical processes. We investigate regimes of decaying high-speed molecular turbulence. Here we analyse PDFs of density for the volume, mass, molecular mass and the energy distribution over the range of scales. We compare our results to those previously obtained for isothermal turbulence and suggest possible explanations.

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