Pavlovski, G., Smith, M.D., Mac Low, M.-M., Rosen, A. (2004) Hydrodynamical simulations of molecular dynamics in supersonic turbulent flow. Astrophysics and Space Science, 292 (1-4). pp. 69-75. ISSN 0004-640X. (doi:10.1023/B:ASTR.0000045002.62859.14) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:50118)
| The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided. | |
| Official URL: http://dx.doi.org/10.1023/B:ASTR.0000045002.62859.... |
Abstract
Here we present results from simulations of turbulence in starforming 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.
| Item Type: | Article |
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| DOI/Identification number: | 10.1023/B:ASTR.0000045002.62859.14 |
| Uncontrolled keywords: | clouds, hydrodynamics, ISM, molecular processes, turbulence |
| Subjects: | Q Science > QB Astronomy > QB460 Astrophysics |
| Divisions: | Divisions > Division of Natural Sciences > Physics and Astronomy |
| Depositing User: | Giles Tarver |
| Date Deposited: | 11 Aug 2015 09:40 UTC |
| Last Modified: | 16 Nov 2021 10:20 UTC |
| Resource URI: | https://kar.kent.ac.uk/id/eprint/50118 (The current URI for this page, for reference purposes) |
University of Kent Author Information
Smith, M.D..
| Creator's ORCID: |
 https://orcid.org/0000-0002-4289-5952
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