Metal abundances in the ICM as a diagnostics of the cluster history

Advances in Space Research

Volumn 36, Issue 4, 2005, Pages 677-681

  Bohringer H ^a   Matsushita, K ^b   Finoguenov, A ^a   Xue, Y ^c   Churazov, E ^d  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b TOKYO UNIVERSITY OF SCIENCE   (Japan)

^c CHINESE ACADEMY OF SCIENCES   (China)

^d MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Abundances; Chemical composition (97.10.Tk); Elliptical galaxies (98.54.Ew); Galaxy clusters (98.65.Cw)

Indexed keywords

ASTROPHYSICS; COMPOSITION; COOLING SYSTEMS; HEAVY METALS; METALLIZING;

ABUNDANCES; COOLING CORE; ELLIPTICAL GALAXIES (98.54.EW); GALAXY CLUSTERS (98.65.CW);

GALAXIES;

EID: 27744559299     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.asr.2005.01.096     Document Type: Conference Paper

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