The radial dependence of temperature and iron abundance - Galaxy clusters from z = 0.14 to z = 0.89

Astronomy and Astrophysics

Volumn 503, Issue 1, 2009, Pages 35-46

  Ehlert, S ^a,c   Ulmer, M P ^b,c  

^a MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^b AIX MARSEILLE UNIVERSITÉ   (France)

^c NORTHWESTERN UNIVERSITY   (United States)

Author keywords

X rays: galaxies: clusters

Indexed keywords

ABUNDANCE-GALAXY; ARCHIVAL DATA; CHANDRA; CLUSTER SURVEY; CLUSTERS OF GALAXIES; COSMOLOGICAL PARAMETERS; GALAXY CLUSTERS; HIERARCHICAL STRUCTURES; HIGH-REDSHIFT; INTRA-CLUSTER MEDIUM; LOCAL ENVIRONMENTS; PRIMARY SOURCES; RADIAL PROFILES; RED SHIFT; X RAYS: GALAXIES: CLUSTERS; XMM-NEWTON;

BIOLOGY; COSMOLOGY; GRAVITATION; HEATING;

GALAXIES;

EID: 77952903150     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200809809     Document Type: Article

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