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Astronomy and Astrophysics Supplement Series, Vol. 119, October II 1996, 321-328
Spectroscopic analysis of 31 Aquilae
T.V. Mishenina
Astronomical Observatory, Odessa State University, Odessa 270014, Ukraine
Received June 12, 1995; accepted March 21, 1996
Abstract:
31 Aquilae is the only evolved star for which SMR status was confirmed by Taylor (1991). For this reason, a new determination of the atmospheric parameters and chemical composition of 31 Aql has been made. The observational material consists of high-dispersion coudé echelle spectra obtained with a CCD detector and the 1-m telescope of the Special Observatory of the Russian Academy of Sciences. The new value of [Fe/H] obtained here is +0.32
dex. This is close to
the upper limit of [Fe/H] for dwarf stars belonging to the thin
disk of the Galaxy. The value of the Li abundance 
A(Li)
= 1.35. The value [
] obtained here is 
dex.
Within the errors, solar values of [element/Fe] are obtained for
Na, Y, Zr, Ba, La, Ce, Pr, and Nd. The age of 31 Aql and its
location in the Galaxy are estimated, and a careful analysis of
abundance determination errors is carried out. 31 Aql is found
to be in the evolutionary stage in which the convective envelope
begins to extend.
Key words: stars: abundances --- stars: evolution --- stars: 31 Aql
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