An XMM-Newton spatially-resolved study of metal abundance evolution in distant galaxy clusters

Astronomy and Astrophysics

Volumn 537, Issue , 2012, Pages

  Baldi, A ^a,b   Ettori, S ^b,c   Molendi, S ^d   Balestra, I ^e   Gastaldello, F ^d,f   Tozzi, P ^g,h  

^a UNIVERSITY OF BOLOGNA   (Italy)

^b OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^c INFN SEZIONE DI BOLOGNA   (Italy)

^d INAF IASF MILANO   (Italy)

^e MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^h SEZIONE DI TRIESTE   (Italy)

Author keywords

galaxies: clusters: intracluster medium; X rays: galaxies: clusters

Indexed keywords

CLUSTERS OF GALAXIES; CONFIDENCE LEVELS; DATA POINTS; EMISSION MEASUREMENT; ERROR BARS; EVOLUTIONARY PATH; GALAXY CLUSTERS; INTRA-CLUSTER MEDIUM; LOW QUALITIES; METAL ABUNDANCES; METALLICITIES; POWER LAW; RED SHIFT; SAMPLE SIZES; SPATIALLY RESOLVED; TEMPERATURE RANGE; THEORETICAL PREDICTION; X RAYS: GALAXIES: CLUSTERS; X-RAY SPECTRA; XMM-NEWTON;

SPECTRUM ANALYSIS;

GALAXIES;

EID: 84856150717     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117836     Document Type: Article

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