Issue |
A&A
Volume 426, Number 1, October IV 2004
|
|
---|---|---|
Page(s) | 37 - 51 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361:20040536 | |
Published online | 05 October 2004 |
Continuous star formation in IZw18
1
Institut für theoretische Physik und Astrophysik, Kiel University, Olshausenstrasse 40, 24118 Kiel, Germany e-mail: recchi@mpa-garching.mpg.de
2
Max-Planck Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85741 Garching bei München, Germany
3
Dipartimento di Astronomia, Università di Trieste, Via GB Tiepolo, 11, 34131 Trieste, Italy e-mail: matteucci@ts.astro.it
4
INAF - Osservatorio Astronomico di Bologna, Via Ranzani 1, 40127 Bologna, Italy e-mail: [annibale;tosi]@bo.astro.it
Received:
27
March
2004
Accepted:
25
May
2004
We study the dynamical and chemical evolution of a galaxy
similar to IZw18 under the assumption of a continuous star formation
during bursts. We adopt a 2-D hydrocode coupled with detailed
chemical yields originating from SNeII, SNeIa and from single
intermediate-mass stars. Different nucleosynthetic yields and
different IMF slopes are tested. In most of the explored cases, a
galactic wind develops, mostly carrying out of the galaxy the
metal-enriched gas produced by the burst itself. The chemical species
with the largest escape probabilities are Fe and N. Consequently, we
predict that the [ α/Fe] and [ α/N] ratios outside the
galaxy are lower than inside. In order to reproduce the chemical
composition of IZw18, the best choice seems to be the adoption of the
yields of Meynet & Maeder ([CITE]) which take into account stellar
rotation, although these authors do not follow the whole evolution of
all the stars. Models with a flat IMF () seem to be able to
better reproduce the chemical properties of IZw18, but they inject in
the gas a much larger amount of energy and the resulting galactic wind
is very strong, at variance with observations. We also predict the
evolution of the abundances in the H i medium and compare them with
recent FUSE observations.
Key words: hydrodynamics / ISM: abundances / ISM: jets and outflows / galaxies: evolution / galaxies: individual: IZw18 / galaxies: spiral
© ESO, 2004
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