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  Angular fluctuations in the CXB: is Fe 6.4 keV line tomography of the large-scale structure feasible?

Hütsi, G., Gilfanov, M., & Sunyaev, R. (2012). Angular fluctuations in the CXB: is Fe 6.4 keV line tomography of the large-scale structure feasible? Astronomy & Astrophysics, 547: A21, pp. 1-12. doi:10.1051/0004-6361/201219796.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-000E-7862-9 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0028-4BEB-4
Genre: Journal Article

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 Creators:
Hütsi, G.1, Author              
Gilfanov, M.1, Author              
Sunyaev, R.1, Author              
Affiliations:
1High Energy Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159881              

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Language(s): eng - English
 Dates: 2012-11
 Publication Status: Published in print
 Pages: -
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 Rev. Method: Peer
 Identifiers: DOI: 10.1051/0004-6361/201219796
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Title: Astronomy & Astrophysics
  Abbreviation : Astron. Astrophys.
Source Genre: Journal
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Pages: - Volume / Issue: 547 Sequence Number: A21 Start / End Page: 1 - 12 Identifier: ISSN: 0004-6361