Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-02-10
Astron.Astrophys. 416 (2004) L21
Astronomy and Astrophysics
Astrophysics
5 pages, 4 figures, A&A in press. Astronomy and Astrophysics Letters, in press
Scientific paper
10.1051/0004-6361:20040047
Recent XMM-Newton observations of clusters of galaxies have provided detailed information on the distribution of heavy elements in the central regions of clusters with cooling cores providing strong evidence that most of these metals come from recent SN type Ia. In this paper we compile information on the cumulative mass profiles of iron, the most important metallicity tracer. We find that long enrichment times (larger than 5 Gyr) are necessary to produce the central abundance peaks. Classical cooling flows, a strongly convective intracluster medium, and a complete metal mixing by cluster mergers would destroy the observed abundance peaks too rapidly. Thus the observations set strong constraints on cluster evolution models requiring that the cooling cores in clusters are preserved over very long times. We further conclude from the observations that the innermost part of the intracluster medium is most probably dominated by gas originating predominantly from stellar mass loss of the cD galaxy.
Boehringer Hans
Churazov Eugene
Finoguenov Alexis
Ikebe Yasushi
Matsushita Kyoko
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