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Signatures of Turbulence in the Dense Interstellar Medium

Falgarone, E. and Phillips, T. G. (1991) Signatures of Turbulence in the Dense Interstellar Medium. In: Fragmentation of Molecular Clouds and Star Formation. International Astronomical Union Symposium (IAUS). No.147. Springer Netherlands , Dordrecht, pp. 119-136. ISBN 9780792311591. https://resolver.caltech.edu/CaltechAUTHORS:20201023-182805415

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Abstract

We present an ensemble of recent observational results on molecular clouds which, taken separately, could all be understood by invoking various unrelated physical processes, but taken all together form a coherent ensemble stressing the imprints of turbulence in the physics of the cold interstellar medium. These results are first, the existence of wings in the molecular line profiles, which can be interpreted on statistical grounds as the signature of the intermittency of the velocity field in turbulent flows, second the fractal geometry of the cloud edges, with properties reminiscent of those of various surfaces studied in turbulent laboratory flows, and third, the fact that the dense gas fills only a very small fraction of the space. The last points are supported by CO multitransition observations of a few fields in nearby molecular clouds. They show that the excitation conditions are the same for the gas emitting in the linewings and in the linecores and are also remarkably uniform over a large range (factor 10) of column densities. An attractive interpretation of the molecular line data is that most of the ¹²CO(J=2−l) and (J=3−2) emissions arise in cold (T_k ≤ 10K) and dense (ⁿH₂ ~ 10⁴ cm⁻³ or more) structures distributed on a fractal set with no characteristic scale size greater than about 1000 AU.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/978-94-011-3384-5_15DOIArticle
https://rdcu.be/b9me5PublisherFree ReadCube access
Additional Information:© Springer Science+Business Media Dordrecht 1991.
Subject Keywords:Molecular clouds, Turbulence, Intermittency, Linewings, Fractal structure, Self-similarity
Series Name:International Astronomical Union Symposium (IAUS)
Issue or Number:147
DOI:10.1007/978-94-011-3384-5_15
Record Number:CaltechAUTHORS:20201023-182805415
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20201023-182805415
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:106272
Collection:CaltechAUTHORS
Deposited By: Rebecca Minjarez
Deposited On:29 Oct 2020 19:13
Last Modified:16 Nov 2021 18:52

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