Turbulence in molecular clouds - A new diagnostic tool to probe their origin

Details Turbulence in molecular clouds - A new diagnostic tool to probe their origin Turbulence in molecular clouds - A new diagnostic tool to probe their origin

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...294l.125c&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 294, July 15, 1985, p. L125-L129. NASA-supported re

Statistics

Computation

9

Interstellar Matter, Molecular Clouds, Turbulence, Computational Astrophysics

Scientific paper

A method is presented to uncover the instability responsible for the type of turbulence observed in molecular clouds and the value of the physical parameters of the 'placental medium' from which turbulence originated. The method utilizes the observational relation between velocities and sizes of molecular clouds, together with a recent model for large-scale turbulence (constructed by Canuto and Goldman, 1985).

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