Galaxy-cluster gas-density distributions of the representative XMM-Newton cluster structure survey (REXCESS)

Astronomy and Astrophysics

Volumn 487, Issue 2, 2008, Pages 431-443

  Croston, J H ^a   Pratt, G W ^b   Bohringer H ^b   Arnaud, M ^c   Pointecouteau, E ^d   Ponman, T J ^e   Sanderson, A J R ^e   Temple, R F ^e   Bower, R G ^f   Donahue, M ^g  

^a UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c UNIVERSITÉ PARIS DIDEROT   (France)

^d IRAP   (France)

^e UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^f DURHAM UNIVERSITY   (United Kingdom)

^g MICHIGAN STATE UNIVERSITY   (United States)

Author keywords

Cosmology: large scale structure of Universe; Galaxies: clusters: general; Galaxies: intergalactic medium

Indexed keywords

CHLORINE COMPOUNDS; COSMOLOGY; GASES; IMAGE SEGMENTATION; OPTICAL PROPERTIES; SURVEYS;

COSMOLOGY: LARGE-SCALE STRUCTURE OF UNIVERSE; DENSITY DISTRIBUTIONS; DENSITY PROFILES; GALAXIES: CLUSTERS: GENERAL; GALAXIES: INTERGALACTIC MEDIUM; GAS DISTRIBUTIONS; INTRA-CLUSTER MEDIUM; NON-PARAMETRIC; REPRESENTATIVE XMM-NEWTON CLUSTER STRUCTURE SURVEY; SAMPLING STRATEGIES; SCALING PROPERTIES; SURFACE BRIGHTNESSES; TEMPERATURE RANGES; X-RAY LUMINOSITIES; XMM-NEWTON;

DENSITY OF GASES;

EID: 48849087991     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20079154     Document Type: Article

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