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  Dynamical difference between the cD galaxy and the diffuse, stellar component in simulated galaxy clusters

Dolag, K., Murante, G., & Borgani, S. (2010). Dynamical difference between the cD galaxy and the diffuse, stellar component in simulated galaxy clusters. Monthly Notices of the Royal Astronomical Society, 405(3), 1544-1559. doi:10.1111/j.1365-2966.2010.16583.x.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0012-C54A-C Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0012-C54C-8
Genre: Journal Article

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 Creators:
Dolag, K.1, Author           
Murante, G., Author
Borgani, S., Author
Affiliations:
1Cosmology, MPI for Astrophysics, Max Planck Society, Garching, DE, ou_159876              

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Language(s): eng - English
 Dates: 2010-07-01
 Publication Status: Issued
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 Rev. Type: Peer
 Identifiers: DOI: 10.1111/j.1365-2966.2010.16583.x
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Title: Monthly Notices of the Royal Astronomical Society
  Alternative Title : Mon. Not. R. Astr. Soc.
Source Genre: Journal
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Pages: - Volume / Issue: 405 (3) Sequence Number: - Start / End Page: 1544 - 1559 Identifier: ISSN: 0035-8711