2012A&A...546A..90B


Query : 2012A&A...546A..90B

2012A&A...546A..90B - Astronomy and Astrophysics, volume 546A, 90-90 (2012/10-1)

NLTE analysis of sr lines in spectra of late-type stars with new R-matrix atomic data.

BERGEMANN M., HANSEN C.J., BAUTISTA M. and RUCHTI G.

Abstract (from CDS):

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

Abstract Copyright:

Journal keyword(s): atomic data - line: formation - radiative transfer - Sun: abundances - stars: abundances - stars: atmospheres

VizieR on-line data: <Available at CDS (J/A+A/546/A90): data will be available with accompanying paper>

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
#notes
1 * alf CMi SB* 07 39 18.11950 +05 13 29.9552 0.82 0.79 0.37 -0.05 -0.28 F5IV-V+DQZ 1825 0
2 HD 122563 Pe* 14 02 31.8455084952 +09 41 09.944391876 7.47 7.10 6.19 5.37 4.79 G8:III:Fe-5 800 0
3 * alf Boo RG* 14 15 39.67207 +19 10 56.6730 2.46 1.18 -0.05 -1.03 -1.68 K1.5IIIFe-0.5 2232 0

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2022.08.15-15:16:19

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