Chandra observations of the cooling flow cluster Abell 1835

Details Chandra observations of the cooling flow cluster Abell 1835 Chandra observations of the cooling flow cluster Abell 1835

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000head....5.1317s&link_type=abstract

American Astronomical Society, HEAD Meeting #5, #13.17; Bulletin of the American Astronomical Society, Vol. 32, p.1200

Astronomy and Astrophysics

Astronomy

Scientific paper

We present the analysis of Chandra observations of the massive galaxy cluster Abell 1835. The high spatial resolution of Chandra enables us to study in detail variations of the X-ray spectrum with radius from the central cooling flow out to radii of a Megaparsec. In particular, we can measure the mass deposition rate and the excess absorption in the cooling flow as a function of radius. In the cluster core we find evidence for substructure of the X-ray emission on scales of several kiloparsecs.

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