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A&A 463, L1-L4 (2007)
DOI: 10.1051/0004-6361:20066878
Letter
First detection of photospheric depletion in the Large Magellanic Cloud
M. Reyniers and H. Van WinckelInstituut voor Sterrenkunde, Departement Natuurkunde en Sterrenkunde, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
e-mail: maarten@ster.kuleuven.be
(Received 5 December 2006 / Accepted 31 December 2006 )
Abstract
Context.Recent photospheric abundance studies of galactic field RV Tauri stars show
that depletion of refractory elements is rather common in these evolved
objects.
Aims.The process that creates this chemical anomaly is not understood well, but
it probably requires the presence of gravitationally bound dust in a binary
system. We test for the presence of depletion in extra-galactic objects.
Methods.A detailed photospheric abundance study on the basis of high-quality
UVES spectra was performed on the RV Tauri star in the LMC:
MACHO 82.8405.15.
Abundances were derived using a critically compiled line list with
accurate log(gf) values and the latest Kurucz model atmospheres.
Results.With [Fe/H] = -2.6 in combination with [Zn/Fe] = +2.3 and
[S/Ti] = +2.5, MACHO 82.8405.15 displays a strong depletion abundance
pattern. The effect of the depletion is comparable to the strongest
depletions seen in field Galactic RV Tauri stars.
Conclusions.The chemical analysis of MACHO 82.8405.15 proves that the depletion process
also occurs in the extragalactic members of the RV Tauri pulsation class. Our
program star is a member of a larger sample of LMC RV Tauri objects. This
sample is unique, since the distances of the members are well-constrained.
Further studies of this sample are therefore expected to gain deeper insight
into the poorly understood depletion phenomenon and of the evolutionary status
of RV Tauri stars in general.
Key words: stars: AGB and post-AGB -- stars: abundances -- stars: individual: MACHO 82.8405.15 -- Magellanic Clouds
© ESO 2007
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