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  Turbulent gas motions in galaxy cluster simulations: the role of smoothed particle hydrodynamics viscosity

Dolag, K., Vazza, F., Brunetti, G., & Tormen, G. (2005). Turbulent gas motions in galaxy cluster simulations: the role of smoothed particle hydrodynamics viscosity. Monthly Notices of the Royal Astronomical Society, 364(3), 753-772. doi:10.1111/j.1365-2966.2005.09630.x.

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 Creators:
Dolag, K.1, Author           
Vazza, F., Author
Brunetti, G., Author
Tormen, G., Author
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1Cosmology, MPI for Astrophysics, Max Planck Society, ou_159876              

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Language(s): eng - English
 Dates: 2005-12-11
 Publication Status: Issued
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: eDoc: 249233
DOI: 10.1111/j.1365-2966.2005.09630.x
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Title: Monthly Notices of the Royal Astronomical Society
  Alternative Title : Mon. Not. Roy. Astron. Soc.
Source Genre: Journal
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Pages: - Volume / Issue: 364 (3) Sequence Number: - Start / End Page: 753 - 772 Identifier: ISSN: 1364-8711
ISSN: 0035-8711