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

Y.-Y. Zhang; T. F. Laganá; D. Pierini; E. Puchwein; P. Schneider; T. H. Reiprich

doi:10.1051/0004-6361/201116803e

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Volume 544 (August 2012)

A&A, 544 (2012) C3

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Issue		A&A Volume 544, August 2012


Article Number		C3
Number of page(s)		1
Section		Cosmology (including clusters of galaxies)
DOI		https://doi.org/10.1051/0004-6361/201116803e
Published online		21 August 2012

A&A 544, C3 (2012)

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

Y.-Y. Zhang¹^,2, T. F. Laganá³^,1, D. Pierini⁴^,⋆, E. Puchwein⁵^,6, P. Schneider¹ and T. H. Reiprich¹

¹ Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
e-mail: yyzhang@astro.uni-bonn.de
² National Astronomical Observatories, Chinese Academy of Sciences, 100012 Beijing, PR China
³ Universidade de São Paulo, Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Departamento de Astronomia, Rua do Matão 1226, Cidade Universitária, CEP: 05508-090, São Paulo, SP, Brasil
⁴ Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, 85748 Garching, Germany
⁵ Heidelberger Institut für Theoretische Studien, Schloss-Wolfsbrunnenweg 35, 69118 Heidelberg, Germany
⁶ Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Straße 1, 85741 Garching, Germany

Key words: cosmology: observations / galaxies: clusters: general / methods: data analysis / surveys / X-rays: galaxies: clusters / errata, addenda

^⋆

Guest astronomer at the MPE.

In our original paper, we inadvertently tabulated the stellar masses from a Kroupa (2001) initial mass function in Table 1, which are not consistent with the remaining content of the paper. We note that this does not affect any of our results. Nevertheless, we regret this error and provide the actual stellar masses in Table 1 from a Salpeter (1955) initial mass function.

Table 1

Properties of the 19 galaxy clusters.

Acknowledgments

The authors would like to thank Anthony Gonzalez for pointing out this error in our manuscript.

References

Kroupa, P. 2001, MNRAS, 322, 231 [NASA ADS] [CrossRef] [Google Scholar]
Salpeter, E. E. 1955, ApJ, 121, 161 [NASA ADS] [CrossRef] [Google Scholar]

© ESO, 2012

All Tables

Table 1

Properties of the 19 galaxy clusters.

In the text

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