Skip to main content

The decay of supersonic and super-Alfvenic turbulence in star-forming clouds: The spatial distribution of shocks

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)

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. (Contact us about this Publication)
Official URL
http://dx.doi.org/10.1023/A:1002036113496

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
DOI/Identification number: 10.1023/A:1002036113496
Subjects: Q Science > QB Astronomy > QB460 Astrophysics
Divisions: Faculties > Sciences > School of Physical Sciences > Centre for Astrophysics and Planetary Sciences
Depositing User: Giles Tarver
Date Deposited: 11 Aug 2015 10:22 UTC
Last Modified: 29 May 2019 15:55 UTC
Resource URI: https://kar.kent.ac.uk/id/eprint/50142 (The current URI for this page, for reference purposes)
  • Depositors only (login required):