An Orientation of Rich Clusters and the Brightest Cluster Members for MRSS Clusters

Details An Orientation of Rich Clusters and the Brightest Cluster Members for MRSS Clusters An Orientation of Rich Clusters and the Brightest Cluster Members for MRSS Clusters

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confe..75p&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 75-75"

Computer Science

Scientific paper

Using the Muenster Red Sky Survey being a survey complete till rF=18.3 and covering 5000 square degrees on the southern celestial sphere, applying Voronoi tessellation, we found structures having at least 10 members. Taking into account only rich structures with more than 50 members seen in projection we compare the orientation of the position angles of the brightest cluster member with the position angle of the cluster itself.

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