Bibcode
Lemasle, B.; de Boer, T. J. L.; Hill, V.; Tolstoy, E.; Irwin, M. J.; Jablonka, P.; Venn, K.; Battaglia, G.; Starkenburg, E.; Shetrone, M.; Letarte, B.; François, P.; Helmi, A.; Primas, F.; Kaufer, A.; Szeifert, T.
Referencia bibliográfica
Astronomy and Astrophysics, Volume 572, id.A88, 28 pp.
Fecha de publicación:
12
2014
Revista
Número de citas
69
Número de citas referidas
60
Descripción
Context. Fornax is one of the most massive dwarf spheroidal galaxies in
the Local Group. The Fornax field star population is dominated by
intermediate age stars but star formation was going on over almost its
entire history. It has been proposed that Fornax experienced a minor
merger event. Aims: Despite recent progress, only the high
metallicity end of Fornax field stars ([Fe/H] > -1.2 dex) has been
sampled in larger number via high resolution spectroscopy. We want to
better understand the full chemical evolution of this galaxy by better
sampling the whole metallicity range, including more metal poor stars.
Methods: We use the VLT-FLAMES multi-fibre spectrograph in
high-resolution mode to determine the abundances of several α,
iron-peak and neutron-capture elements in a sample of 47 individual red
giant branch stars in the Fornax dwarf spheroidal galaxy. We combine
these abundances with accurate age estimates derived from the age
probability distribution from the colour-magnitude diagram of Fornax.
Results: Similar to other dwarf spheroidal galaxies, the old,
metal-poor stars of Fornax are typically α-rich while the young
metal-rich stars are α-poor. In the classical scenario of the time
delay between Type II (SNe II) and Type Ia Supernovae (SNe Ia), we
confirm that SNe Ia started to contribute to the chemical enrichment at
[Fe/H] between -2.0 and -1.8 dex. We find that the onset of SNe Ia took
place between 12-10 Gyr ago. The high values of [Ba/Fe], [La/Fe] reflect
the influence of SNe Ia and AGB stars in the abundance pattern of the
younger stellar population of Fornax. Conclusions: Our findings
of low [α/Fe] and enhanced [Eu/Mg] are compatible with an initial
mass function that lacks the most massive stars and with star formation
that kept going on throughout the whole history of Fornax. We find that
massive stars kept enriching the interstellar medium in
α-elements, although they were not the main contributor to the
iron enrichment.
Based on FLAMES observations collected at the European Southern
Observatory, proposal number 080.B-0784.Table 7 is only available at the
CDS via anonymous ftp to http://cdsarc.u-strasbg.fr
(ftp://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/572/A88Appendices
are available in electronic form at http://www.aanda.org
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