TURBULENCE SETS THE INITIAL CONDITIONS FOR STAR FORMATION IN HIGH-PRESSURE ENVIRONMENTS

Rathborne, JM, Longmore, SN, Jackson, JM, Kruijssen, JMD, Alves, JF, Bally, J, Bastian, N, Contreras, Y, Foster, JB, Garay, G, Testi, L and Walsh, AJ (2014) TURBULENCE SETS THE INITIAL CONDITIONS FOR STAR FORMATION IN HIGH-PRESSURE ENVIRONMENTS. ASTROPHYSICAL JOURNAL LETTERS, 795 (2). ISSN 2041-8205

Preview

Text 1409.0935v1.pdf - Accepted Version Download (2MB) | Preview

Abstract

Despite the simplicity of theoretical models of supersonically turbulent, isothermal media, their predictions successfully match the observed gas structure
and star formation activity within low-pressure (P=k < 105 K cm

Item Type:	Article
Uncontrolled Keywords:	0201 Astronomical And Space Sciences
Subjects:	Q Science > QB Astronomy
Divisions:	Astrophysics Research Institute
Publisher:	IOP PUBLISHING LTD
Related URLs:	http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000345499000001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=7f77ca1697db64ccb27a8011c7ced90d
Date of acceptance:	1 September 2014
Date of first compliant Open Access:	11 January 2016
Date Deposited:	27 May 2015 13:20
Last Modified:	04 Sep 2021 14:19
DOI or ID number:	10.1088/2041-8205/795/2/L25
URI:	https://researchonline.ljmu.ac.uk/id/eprint/1313

View Item