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Home All issues Volume 508 / No 2 (December III 2009) A&A, 508 2 (2009) 677-693 Full HTML
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Table 6:

Li absorption and H$\alpha $ infilling.
Object $T_{\rm eff}$ $W^{\rm int}_{\rm Li}$ $W^{\rm fit}_{\rm Li}$ $W^{{\rm KS05}}_{\rm Li}$ $\log N^{\rm cog}_{\rm LTE}({\rm Li})$ $\log N^{\rm cog}_{\rm NLTE}({\rm Li})$ $\log N^{\rm fit}_{\rm LTE}({\rm Li})$ $\log N^{\rm KS05}_{\rm LTE}({\rm Li})$ H$\alpha $ core $F_{\rm H\alpha }$ [105 erg cm-2 s-1]
  [K] [mÅ] [mÅ] [mÅ]         [%]  
M01k      
HD 11131 5796c 70.5 $\pm$ 1.9 71.2 78.0 2.47 $\pm$ 0.06 2.46 $\pm$ 0.06 2.58 $\pm$ 0.10 2.38 $\pm$ 0.04 29c 10.87
HD 24916 A 4600b <8.0 $\pm$ 3.0             33 1.08
HD 26923 5975c 88.0 $\pm$ 2.1 88.9 84.3 2.77 $\pm$ 0.07 2.72 $\pm$ 0.06 2.83 $\pm$ 0.09 2.69 $\pm$ 0.03 25c 9.02
HD 38393 6310 65.3 $\pm$ 0.7 63.5 58.5 2.87 $\pm$ 0.05 2.81 $\pm$ 0.04 2.96 $\pm$ 0.09 2.82 $\pm$ 0.03 17 0.33
HD 41593 5278c 14.0 $\pm$ 3.9 15.8   1.17 $\pm$ 0.16 1.29 $\pm$ 0.15 1.20 $\pm$ 0.12   30c 8.72
HD 238087 4350g <20.0 $\pm$ 5.0             39 -
HD 112196 6110 109.8 $\pm$ 3.1 109.5   3.04 $\pm$ 0.06 2.94 $\pm$ 0.05 3.09 $\pm$ 0.09   28 11.17
HD 152863 Aa 4980e <7.0 $\pm$ 5.0             17 -0.37
HD 155674 A $\lesssim$4800 <9.0 $\pm$ 6.0             37 11.87
HD 155674 B 3900f <10.0 $\pm$ 2.0             39 -
HD 167389 5895 59.7 $\pm$ 2.4 59.2 58.8 2.48 $\pm$ 0.08 2.46 $\pm$ 0.07 2.50 $\pm$ 0.10 2.41 $\pm$ 0.04 21 4.70
HD 184960 6310 60.5 $\pm$ 1.9 60.0 61.6 2.82 $\pm$ 0.04 2.76 $\pm$ 0.04 2.90 $\pm$ 0.08 2.78 $\pm$ 0.03 17 -0.02
HD 205435a 5060g <15.0 $\pm$ 5.0             20 -0.73
M01k, K03k      
HD 238224 4350f <11.0 $\pm$ 4.0             61 -
M01k, K03k, K03f      
HD 59747 5094c 35.8 $\pm$ 4.4 38 41.0 1.39 $\pm$ 0.12 1.53 $\pm$ 0.10 1.44 $\pm$ 0.16 1.16 $\pm$ 0.07 32c 9.90
HD 109647 4980 46.0 $\pm$ 5.0 44.2 25.0 1.37 $\pm$ 0.09 1.53 $\pm$ 0.08 1.36 $\pm$ 0.11 0.49 $\pm$ 0.15 34 11.65
HD 110463 4940 21.8 $\pm$ 2.6 23.7 18.0 0.99 $\pm$ 0.11 1.17 $\pm$ 0.10 1.05 $\pm$ 0.11 0.31 $\pm$ 0.06 32 10.03
HD 115043 5850 94.0 $\pm$ 6.0 84.0 101 2.70 $\pm$ 0.08 2.66 $\pm$ 0.06 2.78 $\pm$ 0.11 2.61 $\pm$ 0.08 27 9.48
K03k, K03f      
HD 28495 5465 69.0 $\pm$ 2.4 72.8 71.5 2.14 $\pm$ 0.09 2.18 $\pm$ 0.07 2.21 $\pm$ 0.08 1.86 $\pm$ 0.05 42 20.43
HD 39587 5920c 103.6 $\pm$ 4.4 104.7 102.8 2.83 $\pm$ 0.08 2.77 $\pm$ 0.07 2.91 $\pm$ 0.10 2.74 $\pm$ 0.02 28c 11.14
HD 71974 A 5570 68.0 $\pm$ 4.0 66.7           32 12.90
HD 95650 3634d <45.0 $\pm$ 5.0             73 -
HD 109011 5000 29.0 $\pm$ 6.0 25.9 23.4 1.19 $\pm$ 0.16 1.35 $\pm$ 0.14 1.22 $\pm$ 0.20 0.55 $\pm$ 0.04 36 12.54
HD 171746 A 6100 84.9 $\pm$ 3.5 83.3   2.85 $\pm$ 0.08 2.79 $\pm$ 0.07 2.90 $\pm$ 0.10   17 10.34
HD 171746 B 6040 50.0 $\pm$ 5.0 45.3   2.51 $\pm$ 0.09 2.48 $\pm$ 0.08 2.51 $\pm$ 0.11   27 7.26

(2) Effective temperature is adopted from Table 5 if available, or from other sources as indicated in the footnotes to the table. (3) Equivalent width $W^{\rm int}_{\rm Li}$ of Li I $~{\lambda}6707.8~{\AA}$ from direct integration of the observed profile. (4) Equivalent width $W^{\rm fit}_{\rm Li}$ from fitting with synthetic line profiles. (5) Equivalent width $W^{{\rm KS05}}_{\rm Li}$ according to King & Schuler (2005). (6) Li abundance $\log N^{\rm cog}_{\rm LTE}({\rm Li})$ using $W^{\rm int}_{\rm Li}$ by interpolation of the curves of growth of Soderblom et al. (1993a). (7) After application of the non-LTE corrections of Carlsson et al. (1994) ( $\log N^{\rm cog}_{\rm NLTE}({\rm Li})$). (8) Li abundance $\log N^{\rm fit}_{\rm LTE}({\rm Li})$ derived by fitting a synthetic profile to the observed feature. (9) Li abundance $\log N^{\rm KS05}_{\rm LTE}({\rm Li})$ according to King & Schuler (2005). (10) Relative infilling of the core of H$\alpha $ measured according to Fuhrmann04. (11) Chromospheric flux $F_{\rm H\alpha }$ measured according to Lyra & Porto de Mello (2005).
a Giant. b From König et al. (2006). c From Fuhrmann04. d From Alonso et al. (1996). e From de Laverny et al. (2003). f Converted from spectral type with the calibration from Kenyon & Hartmann (1995). g From McWilliam (1990).


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