Mac Low, M.-M., Smith, M.D., Klessen, R.S., Burkert, A. (1998) The decay of supersonic and super-Alfvenic turbulence in star-forming clouds: The spatial distribution of shocks. Astrophysics and Space Science, 261 (1-4). pp. 195-196. ISSN 0004-640X. (doi:10.1023/A:1002036113496) (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:50142)
| 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/A:1002036113496 |
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| Additional URLs: |
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Abstract
Supersonic and super-Alfvenic turbulent motions generate an intricate pattern of shock waves through which the turbulence decays. We here illustrate the spatial structure during shock formation and decay.
| Item Type: | Article |
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| DOI/Identification number: | 10.1023/A:1002036113496 |
| Subjects: | Q Science > QB Astronomy > QB460 Astrophysics |
| Institutional Unit: | Schools > School of Engineering, Mathematics and Physics > Physics and Astronomy |
| Former Institutional Unit: |
Divisions > Division of Natural Sciences > Physics and Astronomy
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| Depositing User: | Giles Tarver |
| Date Deposited: | 11 Aug 2015 10:22 UTC |
| Last Modified: | 20 May 2025 09:39 UTC |
| Resource URI: | https://kar.kent.ac.uk/id/eprint/50142 (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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