The Cooling Flow in A1795

Details The Cooling Flow in A1795 The Cooling Flow in A1795

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..311f&link_type=abstract

Chandra Proposal ID #01800010

Physics

Chandra Proposal Id #01800010

Scientific paper

To determine the structural and spectral properties of the cooling flow
in the cluster A1795 (Allen & Fabian, MN, 286, 583, 1997; Fabian et
al ApJ, 436, L63, 1994). The use of both FI and BI spectra should enable
the level of excess absorption and its covering factor to be well
quantified.

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