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