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(Reference retrieved automatically from Web of Science through information on FAPESP grant and its corresponding number as mentioned in the publication by the authors.)

Star-formation efficiency and metal enrichment of the intracluster medium in local massive clusters of galaxies

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Author(s):
Zhang, Y. -Y. [1, 2] ; Lagana, T. F. [1, 3] ; Pierini, D. [4] ; Puchwein, E. [5, 6] ; Schneider, P. [1] ; Reiprich, T. H. [1]
Total Authors: 6
Affiliation:
[1] Univ Bonn, Argelander Inst Astron, D-53121 Bonn - Germany
[2] Chinese Acad Sci, Natl Astron Observ, Beijing 100012 - Peoples R China
[3] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, Dept Astron, BR-05508090 Sao Paulo - Brazil
[4] Max Planck Inst Extraterr Phys, D-85748 Garching - Germany
[5] Max Planck Inst Astrophys, D-85741 Garching - Germany
[6] Heidelberger Inst Theoret Studien, D-69118 Heidelberg - Germany
Total Affiliations: 6
Document type: Journal article
Source: Astronomy & Astrophysics; v. 535, NOV 2011.
Web of Science Citations: 26
Abstract

We have investigated the baryon-mass content in a subsample of 19 clusters of galaxies extracted from the X-ray flux-limited sample HIFLUGCS according to their positions in the sky. For these clusters, we measured total masses and characteristic radii on the basis of a rich optical spectroscopic data set, the physical properties of the intracluster medium (ICM) using XMM-Newton and ROSAT X-ray data, and total (galaxy) stellar masses utilizing the SDSS DR7 multi-band imaging. The observed (hot) gas-mass fractions are almost constant in this mass range. We confirm that the stellar mass fraction decreases as the total mass increases and shows (20 +/- 4)% scatter; in addition, we show that it decreases as the central entropy increases. The latter behavior supports a twofold interpretation, where heating from merging quenches the star-formation activity of galaxies in massive systems, and feedback from supernovae and/or radio galaxies drives a significant amount of gas to the regions beyond r(500) or, alternatively, a substantially large amount of intracluster light (ICL) is associated with galaxies in nonrelaxed systems. Furthermore, less massive clusters are confirmed to host less gas per unit total mass; however, they exhibit higher mass fractions in metals, so that their ICM is more metal-rich. This again supports the interpretation that in the potential wells of low-mass systems the star-formation efficiency of galaxies was high or, alternatively, some gas is missing from the hot phase of the ICM. The former hypothesis is preferred as the main driver of the mass-dependent metal enrichment since the total mass-to-optical luminosity ratio increases as the total mass increases. (AU)

FAPESP's process: 08/04318-7 - Intracluster gas enrichment and star formation efficiency in clusters of galaxies
Grantee:Tatiana Ferraz Laganá
Support type: Scholarships in Brazil - Post-Doctorate
FAPESP's process: 06/56213-9 - New physics from space: formation and evolution of structures in the universe
Grantee:Claudia Lucia Mendes de Oliveira
Support type: Research Projects - Thematic Grants