Physics
Scientific paper
Sep 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop...24h&link_type=abstract
Chandra Proposal ID #01800257
Physics
Chandra Proposal Id #01800257
Scientific paper
The next major step in our understanding of the hydrodynamics of cluster evolution will come from 2-dimensional abundance maps: unobtainable with ASCA but inevitable with AXAF. We propose A3266 as an ideal cluster in which to study a merging system using 2-dimension temperature and abundance maps obtained with the ACIS-I. Recent optical studies show a huge "tidal arm and remarkable velocity substructure". ASCA observations suggest that it is in the midst of a spectacular merger.
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