J/A+A/503/541  Neutral Li in late-type stars non-LTE calculations  (Lind+, 2009)

Departures from LTE for neutral Li in late-type stars. Lind K., Asplund M., Barklem P.S. <Astron. Astrophys. 503, 541 (2009)> =2009A&A...503..541L 2009A&A...503..541L
ADC_Keywords: Stars, late-type ; Abundances ; Atomic physics Keywords: stars: abundances - stars: late-type - line: formation Abstract: We perform non-LTE calculations of lithium in late-type stars for a wide range of stellar parameters, including quantum mechanical cross-sections for collisions with neutral hydrogen and the negative hydrogen ion. Non-LTE abundance corrections for the lithium resonance line at 670.7nm and the subordinate line at 610.3nm, are calculated using 1D MARCS model atmospheres spanning a large grid in effective temperature, surface gravity, and metallicity, and lithium abundance. The competing effects of ultraviolet over-ionization and photon losses in the resonance line govern the behaviour of the non-LTE effects with stellar parameters and lithium abundance. The size and sign of the non-LTE abundance corrections vary significantly over the grid for the 670.7nm line, but are typically positive and below 0.15dex for the 610.3nm line. The new collisional data play a significant role in determining the abundance corrections. Description: Non-LTE abundance corrections and equivalent widths for atmospheric models in the stellar parameter range Teff=[4000,8000]K, log(g)=[1.0,5.0], [Fe/H]=[0.0,-3.0], and microturbulence [1.0,5.0]km/s. The lithium abundance ranges between A(Li)=[-0.3,4.2]. An IDL-code for interpolation between table-values can be obtained on request to klind(at)eso.org. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 47 5431 Non-LTE abundance corrections and equivalent widths for the 670.7nm line table3.dat 47 4388 Non-LTE abundance corrections and equivalent widths for the 610.3nm line -------------------------------------------------------------------------------- See also: J/PASJ/57/45 : Lithium abundances of F-K stars (Takeda+, 2005) J/A+A/503/545 : NGC 6397 Li depletion and Li-Na anti-correlation (Lind+, 2009) Byte-by-byte Description of file: table2.dat table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 K Teff Effective temperature 7- 9 F3.1 [cm/s2] logg Surface gravity 12- 15 F4.1 [Sun] [Fe/H] Metallicity 18- 20 F3.1 km/s Vturb Microturbulence velocity 23- 26 F4.1 [Sun] A(Li) LTE lithium abundance 29- 33 F5.2 [Sun] Delta Non-LTE abundance correction (1) 36- 40 F5.2 pm W(LTE) LTE equivalent width 43- 47 F5.2 pm W(NLTE) Non-LTE equivalent width -------------------------------------------------------------------------------- Note (1): Corrections are given for equivalent widths in the range 0.01-100pm. -------------------------------------------------------------------------------- Acknowledgements: Karin Lind, klind(at)eso.org
(End) Karin Lind [ESO, Germany], Patricia Vannier [CDS] 02-Jun-2009
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