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Table · dataset · 2012

NLTE analysis of Sr lines

Listed in IVOA Registry (Virtual Observatory)

We investigate the statistical equilibrium of neutral and singly-ionized strontium in late-type stellar atmospheres.

Description

Particular attention is given to the completeness of the model atom, which includes new energy levels, transition probabilities, photoionization and electron-impact excitation cross-sections computed with the R-matrix method. The NLTE model is applied to the analysis of SrI and SrII lines in the spectra of the Sun, Procyon, Arcturus, and HD 122563, showing a significant improvement in the ionization balance compared to LTE line formation calculations, which predict abundance discrepancies of up to 0.5dex.

The solar Sr abundance is log(epsilon)=2.93+/-0.04dex, in agreement with the meteorites. We present the grid of NLTE abundance corrections for SrI and SrII lines that covers a wide range of stellar parameters. **************************************************************************

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  • The publication of the data will only be postponed until the
  • * accompanying paper is published
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Space sciences 73%
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/546/a9015 d agoJSON v1
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