Search for X-ray signatures of the cosmic web in superclusters

Details Search for X-ray signatures of the cosmic web in superclusters Search for X-ray signatures of the cosmic web in superclusters

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1248..300m&link_type=abstract

X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Confer

Computer Science

Databases

Satellites, Artificial, Clusters Of Galaxies, Sky Surveys, Galaxies, Artificial Earth Satellites, Galaxy Clusters, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc., Protogalaxies, Primordial Galaxies

Scientific paper

We investigated an X-ray selected sample of galaxy clusters in terms of their interactions with the large-scale structure filaments. The analysis was based on the X-ray observations performed by the XMM-Newton satellite over the last 10 years. Nine clusters in the sample of forty show excess emission in the direction of the cosmic web filaments. Since the excess emission is present within the cluster virial radius, we suggest that it is an evidence of the gas moving towards the cluster along the primordial filament.

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