Resolution requirements for simulating gravitational fragmentation using SPH

Hubber, D.A., Goodwin, S.P. and Whitworth, A.P. (2006) Resolution requirements for simulating gravitational fragmentation using SPH. Astronomy and Astrophysics, 450 (3). pp. 881-886. ISSN 0004-6361

Abstract

Metadata

Authors/Creators:
  • Hubber, D.A.
  • Goodwin, S.P.
  • Whitworth, A.P.
Copyright, Publisher and Additional Information: © ESO, 2006. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: stars: formation ; methods: numerical ; hydrodynamics ; instabilities
Dates:
  • Published: May 2006
  • Published (online): 19 April 2006
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield)
Depositing User: Symplectic Sheffield
Date Deposited: 16 Feb 2018 11:43
Last Modified: 16 Feb 2018 11:43
Published Version: https://doi.org/10.1051/0004-6361:20054100
Status: Published
Publisher: EDP Sciences
Refereed: Yes
Identification Number: https://doi.org/10.1051/0004-6361:20054100
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