Galaxy and Cluster Building at Z = 2.4

Details Galaxy and Cluster Building at Z = 2.4 Galaxy and Cluster Building at Z = 2.4

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..696w&link_type=abstract

Chandra Proposal ID #02800623

Physics

Chandra Proposal Id #02800623

Scientific paper

We propose an exploratory Chandra observation of the richest spectroscopically confirmed high-redshift (z>1) galaxy cluster, at z = 2.4. This is the epoch of maximal star formation in galaxies, which is likely to be driving protogalactic winds. Such winds are expected to generate or at least contaminate intracluster gas. We are looking for evidence of diffuse X-ray emission from such winds and/or nascent intracluster gas.

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