An Observational Method to Measure the Relative Fractions of Solenoidal and Compressible Modes in Interstellar Clouds
Autor: | Brunt, C. M., Federrath, C. |
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Rok vydání: | 2014 |
Předmět: | |
Druh dokumentu: | Working Paper |
DOI: | 10.1093/mnras/stu888 |
Popis: | We introduce a new method for observationally estimating the fraction of momentum density (${\rho}{\mathbf{v}}$) power contained in solenoidal modes (for which $\nabla \cdot {\rho}{\mathbf{v}} = 0$) in molecular clouds. The method is successfully tested with numerical simulations of supersonic turbulence that produce the full range of possible solenoidal/compressible fractions. At present the method assumes statistical isotropy, and does not account for anisotropies caused by (e.g.) magnetic fields. We also introduce a framework for statistically describing density--velocity correlations in turbulent clouds. Comment: 20 pages, 13 figures, accepted for publication in MNRAS |
Databáze: | arXiv |
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