Volume 499, Number 3, June I 2009
|Page(s)||891 - 891|
|Published online||25 March 2009|
J. I. González Hernández1,2,3 - R. Rebolo3,4 - G. Israelian3
1 - Observatoire de Paris-Meudon, GEPI, 5 place Jules
Janssen, 92195 Meudon Cedex, France
2 - CIFIST Marie Curie Excellence Team
3 - Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain
4 - Consejo Superior de Investigaciones Científicas, Spain
A&A 478, 203-217 (2008), DOI: 10.1051/0004-6361/20077141
Key words: black holes physics - stars: abundances - stars: individual: Scorpii 1994 (GRO J1655-40) - stars: supernovae: general - X-rays: binaries - errata, addenda
The values of the excitation potential, , and oscillator strength, , of the three lines of the Mg Ib triplet at 5167-83 Å in Table 2 are wrong. The correct values are:
- Mg I 5167.321 Å: eV and
- Mg I 5172.684 Å: eV and
- Mg I 5183.604 Å: eV and .
All the synthetic spectra, as those displayed in Fig. 9, presented in
the paper were computed using the correct values for the excitation
potential and oscillator strengths of these Mg I lines.
Therefore, although we made a mistake in writing the values of and
of these lines in Table 2, the Mg abundances presented
in the paper are also correct.
- ... analysis
- Based on observations obtained with UVES at VLT Kueyen 8.2 m telescope in programme 073.D-0473(A).
Copyright ESO 2009
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