Sheets, filaments, and clumps – high-resolution simulations of how the thermal instability can form molecular clouds

Wareing, CJ orcid.org/0000-0001-9641-0861, Falle, SAEG and Pittard, JM orcid.org/0000-0003-2244-5070 (2019) Sheets, filaments, and clumps – high-resolution simulations of how the thermal instability can form molecular clouds. Monthly Notices of the Royal Astronomical Society, 485 (4). pp. 4686-4702. ISSN 0035-8711

Abstract

Metadata

Authors/Creators:
Copyright, Publisher and Additional Information: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This article has been published in Monthly Notices of the Royal Astronomical Society Published by Oxford University Press on behalf of the Royal Astronomical Society.
Keywords: instabilities; methods: numerical; stars: formation; ISM: clouds; ISM: molecules; ISM: structure
Dates:
  • Published: June 2019
  • Accepted: 6 March 2019
  • Published (online): 14 March 2019
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Maths and Physical Sciences (Leeds) > School of Mathematics (Leeds) > Applied Mathematics (Leeds)
The University of Leeds > Faculty of Maths and Physical Sciences (Leeds) > School of Physics and Astronomy (Leeds) > Astrophysics (Leeds)
Funding Information:
FunderGrant number
Science & Technology Facilities Council (STFC)ST/P00041X/1
Depositing User: Symplectic Publications
Date Deposited: 13 Mar 2019 13:00
Last Modified: 20 May 2019 15:00
Status: Published
Publisher: Oxford University Press
Identification Number: https://doi.org/10.1093/mnras/stz768
Related URLs:

Share / Export

Statistics