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A filament of dark matter between two clusters of galaxies.

Abstract:: It is a firm prediction of the concordance cold-dark-matter cosmological model that galaxy clusters occur at the intersection of large-scale structure filaments. The thread-like structure of this 'cosmic web' has been traced by galaxy redshift surveys for decades. More recently, the warm–hot intergalactic medium (a sparse plasma with temperatures of 10(5) kelvin to 10(7) kelvin) residing in low-redshift filaments has been observed in emission and absorption. However, a reliable direct detecti...
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Publication status:: Published

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APA Style

Dietrich, J., Werner, N., Clowe, D., Finoguenov, A., Kitching, T., Miller, L., & Simionescu, A. (2012). A filament of dark matter between two clusters of galaxies. Nature, 487(7406), 202–204.

MLA Style

Dietrich, J., et al. “A Filament of Dark Matter between Two Clusters of Galaxies.” Nature, vol. 487, no. 7406, 2012, pp. 202–04.

Chicago Style

Dietrich, J, N Werner, D Clowe, A Finoguenov, T Kitching, L Miller, and A Simionescu. 2012. “A Filament of Dark Matter between Two Clusters of Galaxies.” Nature 487 (7406): 202–4.
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Publisher copy:: 10.1038/nature11224

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+ Dietrich, J More by this author

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+ Werner, N More by this author

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+ Clowe, D More by this author

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+ Finoguenov, A More by this author

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+ Kitching, T More by this author

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Bibliographic Details

Journal:: Nature
Volume:: 487
Issue:: 7406
Pages:: 202-204
Publication date:: 2012-07-01
DOI:: 10.1038/nature11224
EISSN:: 1476-4687
ISSN:: 0028-0836

Item Description

Language:: English
Pubs id:: pubs:344024
UUID:: uuid:d0ca08a1-9888-428d-b955-cb0897e7bd50
Local pid:: pubs:344024
Source identifiers:: 344024
Deposit date:: 2012-12-19

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Copyright date:: 2012

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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