The prevalence of cooling cores in clusters of galaxies at z ≈ 0.15-0.4

Monthly Notices of the Royal Astronomical Society

Volumn 359, Issue 4, 2005, Pages 1481-1490

  Bauer, F E ^a,b   Fabian, A C ^a   Sanders, J S ^a   Allen, S W ^a,c   Johnstone, R M ^a  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b Och Spine at New York Presbyterian Hospitals   (United States)

^c STANFORD UNIVERSITY   (United States)

Author keywords

Cooling flows; Galaxies: clusters: general; Surveys; X rays: galaxies: clusters

Indexed keywords

COOLING; GALAXIES; SPECTRUM ANALYSIS;

CHANDRA; CLUSTER OF GALAXIES; COOLING CORE; COOLING FLOWS; COOLING TIME; GALAXIES: CLUSTERS: GENERAL; POWER RATIO; RED SHIFT; TEMPERATURE MAPS; X-RAYS GALAXIES CLUSTERS;

SIGNAL TO NOISE RATIO;

EID: 19844368530     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.08999.x     Document Type: Article

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