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This article is an erratum for: [this article]

Volume 499, Number 3, June I 2009
Page(s) 891 - 891
Section Stellar atmospheres
Published online 25 March 2009


The black hole binary nova Scorpii 1994 (GRO J1655-40): an improved chemical analysis[*]

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, $\chi$, and oscillator strength, $\log gf$, of the three lines of the Mg Ib triplet at 5167-83 Å in Table 2 are wrong. The correct values are:

Mg I $\lambda$5167.321 Å: $\chi=2.709$ eV and $\log gf=-1.03$
Mg I $\lambda$5172.684 Å: $\chi=2.712$ eV and $\log gf=-0.40$
Mg I $\lambda$5183.604 Å: $\chi=2.717$ eV and $\log gf=-0.18$.

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 $\chi$and $\log gf$ 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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