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

Author： Hütsi G.   Gilfanov M.   Sunyaev R.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|547|issue|A21-A21

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.547, Iss.issue, 2012-10, pp. : A21-A21

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