The Chandra Deep Field South: Galaxies and Clusters

Details The Chandra Deep Field South: Galaxies and Clusters The Chandra Deep Field South: Galaxies and Clusters

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000head....5.1404t&link_type=abstract

American Astronomical Society, HEAD Meeting #5, #14.04; Bulletin of the American Astronomical Society, Vol. 32, p.1202

Astronomy and Astrophysics

Astronomy

Scientific paper

We focus on the diffuse X-ray emission from galaxies and clusters of galaxies in the first 300 ksec of exposure of the Chandra Deep Field South. Such an exposure allows to detect diffuse sources down to a surface brightness limit of 5 10-17 erg s-1 cm-2 arcmin-2 in the soft (0.5-2 keV) band. The implications for the thermodynamics of diffuse, hot baryons are discussed.

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