Non-LTE Abundance Analyses of Nitrogen and Sulfur in Chemically Peculiar Stars of the Upper Main Sequence

Astronomy and Astrophysics – Astronomy

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Spectroscopy, Stars: Abundances, Stars: Atmospheres, Stars: Chemically Peculiar Stars, Stars: Early-Type

Scientific paper

The LTE and non-LTE abundances of nitrogen (N) and sulfur (S) in chemically peculiar stars of the upper main sequence were derived from the NI and SI lines observed in a near-infrared spectral region. The sample consisted of 11 stars: three HgMn stars, two Am stars, three magnetic Ap (SrCrEu) stars, two weak-lined stars, and one normal star. The following results were obtained: (1) the LTE abundances of N suffer a large non-LTE effect with correction factors of up to -0.6 dex, while those of S suffer a minor non-LTE effect with correction factors of up to -0.2 dex; (2) the non-LTE abundances of N are systematically below solar value among the sample stars. Although the deficiencies of N are mild in the normal and weak-lined stars, they are enhanced by a factor of up to 2 dex in HgMn stars. A star-to-star variation with a range of 1 dex or more in the N deficiency is shown in Am and SrCrEu stars; (3) the non-LTE abundances of S are solar or slightly overabundant among the sample stars, except for SrCrEu stars. S is systematically deficient relative to the Sun by a factor of >~ 0.7 dex in SrCrEu stars.

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