What we learn about cooling flows through the study of the 10,000 K gas in clusters

Details What we learn about cooling flows through the study of the 10,000 K gas in clusters What we learn about cooling flows through the study of the 10,000 K gas in clusters

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasp..104..848b&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 104, no. 679, p. 848-851.

Astronomy and Astrophysics

Astrophysics

6

Cooling Flows (Astrophysics), Galactic Clusters, Gas Ionization, High Temperature Gases, Nebulae, Emission Spectra, Line Spectra, Physical Properties, X Ray Telescopes

Scientific paper

The physical properties of the emission-line nebulae associated with central dominant galaxies in clusters are explored within the context of standard cooling-flow models of the hot ICM. It is pointed out that the properties of the 10,000 K gas are inconsistent with simple theories in which this gas has accreted out of the hot ICM in thermal instabilities within a standard cooling flow atmosphere. Several possible ramifications for our understanding of the properties of clusters and the hot intracluster medium are discussed.

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