A high-resolution study of the Hydra A cluster with Chandra: Comparison of the core mass distribution with theoretical predictions and evidence for feedback in the cooling flow

Astrophysical Journal

Volumn 557, Issue 2 PART 1, 2001, Pages 546-559

  David, L P ^a   Nulsen, P E J ^b   Mcnamara, B R ^a,c   Forman, W ^a   Jones, C ^a   Ponman, T ^d   Robertson, B ^e   Wise, M ^f  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b UNIVERSITY OF WOLLONGONG   (Australia)

^c OHIO UNIVERSITY   (United States)

^d UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^e UNIVERSITY OF WASHINGTON   (United States)

^f MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Cooling flows; Galaxies: Clusters: Individual (Hydra A); Intergalactic medium; X rays: Galaxies

Indexed keywords

EID: 0035921243     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/322250     Document Type: Article

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