期刊
ASTROPHYSICS AND SPACE SCIENCE
卷 292, 期 1-4, 页码 69-75出版社
SPRINGER
DOI: 10.1023/B:ASTR.0000045002.62859.14
关键词
hydrodynamics; turbulence; molecular processes; clouds; ISM
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.
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