The Decay of Supersonic and Super-Alfvénic Turbulence in Star-Forming Clouds

Authors: Mac Low, M-M.1; Smith, M.D.2; Klessen, R.S.1; Burkert, A.1

Source: Astrophysics and Space Science, Volume 261, Number 1-4, 1998 , pp. 195-196(2)

Publisher: Springer

Buy & download fulltext article:

OR

Price: $47.00 plus tax (Refund Policy)

Abstract:

Supersonic and super-Alfvénic 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.

Document Type: Regular Paper

Affiliations: 1: Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany 2: Astronomisches Institut der Universität Würzburg, Am Hubland, 97074 Würzburg, Germany

Publication date: January 1, 1998

Related content

Key

Free Content
Free content
New Content
New content
Open Access Content
Open access content
Subscribed Content
Subscribed content
Free Trial Content
Free trial content

Text size:

A | A | A | A
Share this item with others: These icons link to social bookmarking sites where readers can share and discover new web pages. print icon Print this page