X-ray Picture of Superclusters of Galaxies

Hudaverdi, M.
Bozkurt, M.
Galaxies gravitationally attract each other and form galaxy groups (similar to 50) or galaxy clusters (> 100). Nevertheless galaxy clusters are not the end of structure formation. Clusters further get together and form Superclusters. Recent studies have shown that the Universe forms cosmic filaments and voids. The superclusters are the intersection points of these filaments. In this work we present an analysis of SCC100 and Shapley supercluster members. Using X-ray data we try to understand the mutual interactions between individual clusters. Since they are the best representatives of the Universe, we try to address large scale properties of the universe.


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Aad, G.; et. al. (2011-12-14)
The Z -> tau tau cross section is measured with the ATLAS experiment at the LHC in four different final states determined by the decay modes of the tau leptons: muon-hadron, electron-hadron, electron-muon, and muon-muon. The analysis is based on a data sample corresponding to an integrated luminosity of 36 pb(-1), at a proton-proton center-of-mass energy of root s = 7 TeV. Cross sections are measured separately for each final state in fiducial regions of high detector acceptance, as well as in the full phas...
Erkurt, A.; Tektunali, H. G.; Hudaverdi, M.; ERCAN, ENİSE NİHAL (2008-10-05)
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Radiative Omega(Q)* -> Omega(Q)gamma and Xi(Q)* -> Xi(Q)'gamma transitions in light cone QCD
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Bozkurt, M.; Hudaverdi, M.; ERCAN, ENİSE NİHAL (2008-10-05)
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Citation Formats
M. Hudaverdi, M. Bozkurt, and E. N. ERCAN, “X-ray Picture of Superclusters of Galaxies,” 2009, vol. 424, p. 330, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/67105.