Hydrodynamical Simulations of Molecular Dynamics in Supersonic Turbulent Flow

  • Georgi Pavlovski
  • Michael D. Smith
  • Mordecai-Mark Mac Low
  • Alexander Rosen


Here we present results from simulations of turbulence in star forming 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.


hydrodynamics turbulence molecular processes clouds ISM 


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Copyright information

© Springer Science+Business Media Dordrecht 2004

Authors and Affiliations

  • Georgi Pavlovski
    • 1
  • Michael D. Smith
    • 1
  • Mordecai-Mark Mac Low
    • 2
  • Alexander Rosen
    • 1
  1. 1.Armagh ObservatoryArmaghN.Ireland, UK
  2. 2.Department of AstrophysicsAmerican Museum of Natural HistoryNew YorkUSA

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