Demonstration Spectrum of a Cooling Flow Cluster: Hydra a

Details Demonstration Spectrum of a Cooling Flow Cluster: Hydra a Demonstration Spectrum of a Cooling Flow Cluster: Hydra a

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cxo..prop..328c&link_type=abstract

Chandra Proposal ID #01800105

Physics

Chandra Proposal Id #01800105

Scientific paper

The radio galaxy Hydra A, is the central dominant galaxy in one of the strongest know cluster cooling flows with a mass accretion rate of 600 Mo/yr. This observation will generate two X-ray spectra (with both a front and back side illuminated ACIS chip) of a cooling flow for science calibration. The Hydra A cluster is also at a low enough redshift (z=0.5) that the central cooling flow region will be resolved with AXAF.

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