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This article is an erratum for: [this article]

Issue A&A
Volume 392, Number 2, September III 2002
Page(s) 489 - 489
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20021095



A&A 392, 489-489 (2002)
DOI: 10.1051/0004-6361:20021095

Erratum

Unusual metal abundances in a pair of damped Lyman alpha systems at $\mathsf{\vec{z} \sim 2}$

S. L. Ellison1 and S. Lopez2

1  European Southern Observatory, Casilla 19001, Santiago 19, Chile
    e-mail: sellison@eso.org
2  Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago, Chile
    e-mail: slopez@das.uchile.cl

(A&A 380, 117-122 (2001), DOI: 10.1051/0004-6361:20011431)

Erratum of A&A  380 p. 117

Abstract
In Table 2 of Ellison & Lopez (2001) the value of [Si/H] in DLA A should be -1.04. Although the subsequent [Si/Fe] is typical of other DLAs, a low ratio of $\alpha$/Fe is still supported by [S/Fe], compared with other systems in the literature. The moderate [Si/Fe] ratio could therefore be due to a modest amount of dust depletion, as supported by [Zn/Cr] = 0.18. If dust is present, this would further decrease the already low [S/Fe] in DLA A. Therefore, despite the revised value of [Si/Fe] in DLA A, these results are still supportive of low $\alpha$/Fe in this double DLA.


Offprint request: S. Ellison, sellison@eso.org



© ESO 2002


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