Chandra Study of the Structure of the Southern Part of the Horologium Supercluster

Details Chandra Study of the Structure of the Southern Part of the Horologium Supercluster Chandra Study of the Structure of the Southern Part of the Horologium Supercluster

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cxo..prop.2030b&link_type=abstract

Chandra Proposal ID #07800645

Astronomy and Astrophysics

Astrophysics

Chandra Proposal Id #07800645

Scientific paper

This proposal is part of a large multi-wavelength effort to characterize the mass distribution and structure of one of the largest known cosmic superstructures, the Horologium Supercluster (SC), and to establish it as an astrophysical laboratory for the study of galaxy and intergalactic medium evolution. The immediate objective of this proposal is the study of the structure and mass of 9 galaxy clusters in the most prominent southern concentration in the SC: to study the connection of cluster and SC structure, the modification of the cluster X-ray luminosity function in the SC, and the constraint reconstruction of the mass distribution in the SC.

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