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- W2095593818 abstract "In this contribution we investigate the connection between clusters of galaxies and their large-scale environment, with an emphasis on clusters which are well characterized by their X-ray emission. We show that this connection is so tight that clusters can be used as perfect tracers of the large-scale matter distribution and thus for cosmological tests. The correlation of the X-ray traced cluster mass and the optical luminosity of the galaxy content of clusters shows that the dark matter and galaxy distribution are tightly connected, but we also observe a scatter which is so far not well understood. We further explore the correlation of the galaxy population mix with the geometry of the large-scale structure features. On larger scales we also find correlations of the properties of galaxy clusters with the density of their large-scale structure environment.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html" @default.
- W2095593818 created "2016-06-24" @default.
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- W2095593818 date "2004-03-01" @default.
- W2095593818 modified "2023-09-26" @default.
- W2095593818 title "X-ray galaxy clusters in the large-scale structure" @default.
- W2095593818 doi "https://doi.org/10.1017/s1743921304000055" @default.
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