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  Modelling self-similar appearance of galaxy clusters in X-rays

Böhringer, H., Dolag, K., & Chon, G. (2012). Modelling self-similar appearance of galaxy clusters in X-rays. Astronomy & Astrophysics, 539: A120, pp. 1-14. doi:10.1051/0004-6361/201118000.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-000F-C33E-C Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0028-4BCB-E
Genre: Journal Article

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 Creators:
Böhringer, H.1, Author              
Dolag, K.2, Author              
Chon, G.3, Author              
Affiliations:
1Theory and Complex Plasmas, MPI for Extraterrestrial Physics, Max Planck Society, ou_159894              
2Cosmology, MPI for Astrophysics, Max Planck Society, ou_159876              
3High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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Language(s): eng - English
 Dates: 2012-03
 Publication Status: Published in print
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 Rev. Method: Peer
 Identifiers: DOI: 10.1051/0004-6361/201118000
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Title: Astronomy & Astrophysics
  Abbreviation : Astron. Astrophys.
Source Genre: Journal
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Pages: - Volume / Issue: 539 Sequence Number: A120 Start / End Page: 1 - 14 Identifier: ISSN: 0004-6361