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A&A 373, 836-842 (2001)
DOI: 10.1051/0004-6361:20010628
Argon, silicon and iron abundances in
the damped Ly-
system I Zw 18
S. A. Levshakov1, W. H. Kegel2 and I. I. Agafonova1
1 Department of Theoretical Astrophysics, Ioffe Physico-Technical Institute, 194021 St. Petersburg, Russia
e-mail: lev@astro.ioffe.rssi.ru
e-mail: ira@astro.ioffe.rssi.ru
2 Insitut für Theoretische Physik der Universität Frankfurt am Main, 60054 Frankfurt/Main 11, Germany
e-mail: kegel@astro.uni-frankfurt.de
(Received 28 November 2000 / Accepted 1 May 2001)
Abstract
We show how the ratio of the abundances of Ar, Si and Fe as derived
from FUSE absorption spectra of I Zw 18 are affected by
large-scale stochastic velocity fields (mesoturbulence).
21-cm observations with high spatial resolution show
the presence of velocity fields with large correlation lengths.
FUSE observations were performed with a large
entrance aperture which fully covered the galaxy.
This means that the observed profiles are averaged over the full
body of I Zw 18.
Taking this into account, we show that
the observations are consistent with the abundance ratios
[
-chain/Fe] being similar to
those derived from Galactic metal-poor stars.
Using a mesoturbulent approach,
we found that
the observed profiles can be reproduced well with
[Fe/H]
, and [Si, Ar/Fe]
.
Key words: line: formation -- line: profiles -- galaxies: individual: I Zw 18
Offprint request: S. A. Levshakov, sergei@oat.ts.astro.it
SIMBAD Objects
© ESO 2001
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