X-Ray Studies of Dynamically Young Clusters of Galaxies

Details X-Ray Studies of Dynamically Young Clusters of Galaxies X-Ray Studies of Dynamically Young Clusters of Galaxies

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1104m&link_type=abstract

Chandra Proposal ID #04800013

Physics

Chandra Proposal Id #04800013

Scientific paper

X-ray linearly flattened clusters may represent an early stage of cluster evolution. With the superior angular-resolution of Chandra, we can search for merger shocks/cold fronts during this stage. Substantial substructures are expected to be found. Moreover, we can study the radio-ICM interaction for A514 and a cooling flow for A2384. The clusters selected help to construct a sample of dynamically young clusters. This sample will eventually help the understanding of cluster formation and early stage of evolution.

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