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A&A 415, 879-884 (2004)
DOI: 10.1051/0004-6361:20034584
Hints of star formation at z
: The
chemical abundances of the DLA system in the QSO BRI 1202-0725 (z
)
V. D'Odorico and P. Molaro INAF - Osservatorio Astronomico di Trieste, via G.B. Tiepolo, 11, 34131 Trieste, Italy
(Received 23 July 2003 / Accepted 30 October 2003 )
Abstract
The Damped Ly-
(DLA) absorber at redshift
observed toward QSO BRI
1202-0725 is studied by means of high resolution
(FWHM
km s
-1) VLT-UVES spectra. We refine
a previously determined Si abundance and derive
with confidence abundances for C, N and O which are
poorly known in DLAs. The [O/Fe] ratio is ~
0.6, but we cannot establish if iron is partially locked into dust grains. The [C/Fe]
and [Si/C]
. [N/O] and [N/Si]
are about
-1, which is consistent with the majority of DLAs.
This value is much larger than the one observed for
the DLA toward QSO J 0307-4945 at
.
The current interpretation of the bimodal distribution of N abundances in DLAs implies that large [ N/
] values correspond to relatively old systems. Adopting a scale time of 500 Myrs for full
N production by intermediate mass stars, the onset of star formation in our DLA took place already at redshift
>
6.
Key words: galaxies: abundances -- galaxies: high-redshift -- galaxies: quasars: absorption lines -- cosmology: observations
Offprint request: V. D'Odorico, dodorico@sissa.it
SIMBAD Objects
© ESO 2004
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